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Albert Einstein

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Albert Einstein[a] (14 March 1879 – 18 April 1955) was a German-born theoretical physicist best known for developing the theory of relativity. Einstein also made important contributions to quantum theory.[1][5] His mass–energy equivalence formula E = mc2, which arises from special relativity, has been called "the world's most famous equation".[6] He received the 1921 Nobel Prize in Physics for "his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect".[7]

Born in the German Empire, Einstein moved to Switzerland in 1895, forsaking his German citizenship (as a subject of the Kingdom of Württemberg)[note 1] the following year. In 1897, at the age of seventeen, he enrolled in the mathematics and physics teaching diploma program at the Swiss federal polytechnic school in Zurich, graduating in 1900. He acquired Swiss citizenship a year later, which he kept for the rest of his life, and afterwards secured a permanent position at the Swiss Patent Office in Bern. In 1905, he submitted a successful PhD dissertation to the University of Zurich. In 1914, he moved to Berlin to join the Prussian Academy of Sciences and the Humboldt University of Berlin, becoming director of the Kaiser Wilhelm Institute for Physics in 1917; he also became a German citizen again, this time as a subject of the Kingdom of Prussia.[note 1] In 1933, while Einstein was visiting the United States, Adolf Hitler came to power in Germany. Horrified by the Nazi persecution of his fellow Jews,[8] he decided to remain in the US, and was granted American citizenship in 1940.[9] On the eve of World War II, he endorsed a letter to President Franklin D. Roosevelt alerting him to the potential German nuclear weapons program and recommending that the US begin similar research, later carried out as the Manhattan Project.

In 1905, sometimes described as his annus mirabilis (miracle year), he published four groundbreaking papers.[10] In them, he outlined a theory of the photoelectric effect, explained Brownian motion, introduced his special theory of relativity, and demonstrated that if the special theory is correct, mass and energy are equivalent to each other. In 1915, he proposed a general theory of relativity that extended his system of mechanics to incorporate gravitation. A cosmological paper that he published the following year laid out the implications of general relativity for the modeling of the structure and evolution of the universe as a whole.[11][12] In 1917, Einstein wrote a paper which introduced the concepts of spontaneous emission and stimulated emission, the latter of which is the core mechanism behind the laser and maser, and which contained a trove of information that would be beneficial to developments in physics later on, such as quantum electrodynamics and quantum optics.[13]

In the middle part of his career, Einstein made important contributions to statistical mechanics and quantum theory. Especially notable was his work on the quantum physics of radiation, in which light consists of particles, subsequently called photons. With physicist Satyendra Nath Bose, he laid the groundwork for Bose–Einstein statistics. For much of the last phase of his academic life, Einstein worked on two endeavors that ultimately proved unsuccessful. First, he advocated against quantum theory's introduction of fundamental randomness into science's picture of the world, objecting that "God does not play dice".[14] Second, he attempted to devise a unified field theory by generalizing his geometric theory of gravitation to include electromagnetism. As a result, he became increasingly isolated from mainstream modern physics.

Life and career

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Childhood, youth and education

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A young boy with short hair and a round face, wearing a white collar and large bow, with vest, coat, skirt, and high boots. He is leaning against an ornate chair.
Einstein in 1882, age 3

Albert Einstein was born in Ulm,[15] in the Kingdom of Württemberg in the German Empire, on 14 March 1879. His parents, secular Ashkenazi Jews, were Hermann Einstein, a salesman and engineer, and Pauline Koch. In 1880, the family moved to Munich's borough of Ludwigsvorstadt-Isarvorstadt, where Einstein's father and his uncle Jakob founded Elektrotechnische Fabrik J. Einstein & Cie, a company that manufactured electrical equipment based on direct current.[15]

When he was very young, his parents worried that he had a learning disability because he was very slow to learn to talk.[16] When he was five and sick in bed, his father brought him a compass. This sparked his lifelong fascination with electromagnetism. He realized that "Something deeply hidden had to be behind things."[17]

Einstein attended St. Peter's Catholic elementary school in Munich from the age of five. When he was eight, he was transferred to the Luitpold Gymnasium, where he received advanced primary and then secondary school education.[18]

Einstein's parents, Hermann and Pauline

In 1894, Hermann and Jakob's company tendered for a contract to install electric lighting in Munich, but without success—they lacked the capital that would have been required to update their technology from direct current to the more efficient, alternating current alternative.[19] The failure of their bid forced them to sell their Munich factory and search for new opportunities elsewhere. The Einstein family moved to Italy, first to Milan and a few months later to Pavia, where they settled in Palazzo Cornazzani.[20] Einstein, then fifteen, stayed behind in Munich in order to finish his schooling. His father wanted him to study electrical engineering, but he was a fractious pupil who found the Gymnasium's regimen and teaching methods far from congenial. He later wrote that the school's policy of strict rote learning was harmful to creativity. At the end of December 1894, a letter from a doctor persuaded the Luitpold's authorities to release him from its care, and he joined his family in Pavia.[21] While in Italy as a teenager, he wrote an essay entitled "On the Investigation of the State of the Ether in a Magnetic Field".[22][23]

Einstein excelled at physics and mathematics from an early age, and soon acquired the mathematical expertise normally only found in a child several years his senior. He began teaching himself algebra, calculus and Euclidean geometry when he was twelve; he made such rapid progress that he discovered an original proof of the Pythagorean theorem before his thirteenth birthday.[24][25] A family tutor, Max Talmud, said that only a short time after he had given the twelve year old Einstein a geometry textbook, the boy "had worked through the whole book. He thereupon devoted himself to higher mathematics ... Soon the flight of his mathematical genius was so high I could not follow."[26] Einstein recorded that he had "mastered integral and differential calculus" while still just fourteen.[27] His love of algebra and geometry was so great that at twelve, he was already confident that nature could be understood as a "mathematical structure".[28]

Studio photo of a boy seated in a relaxed posture and wearing a suit, posed in front of a backdrop of scenery.
Einstein in 1893, age 14

At thirteen, when his range of enthusiasms had broadened to include music and philosophy,[29] Talmud introduced Einstein to Kant's Critique of Pure Reason. Kant became his favorite philosopher; according to Talmud, "At the time he was still a child, only thirteen years old, yet Kant's works, incomprehensible to ordinary mortals, seemed to be clear to him."[26]

In 1895, at the age of sixteen, Einstein sat the entrance examination for the federal polytechnic school (later the Eidgenössische Technische Hochschule, ETH) in Zurich, Switzerland. He failed to reach the required standard in the general part of the test,[30] but performed with distinction in physics and mathematics.[31] On the advice of the polytechnic's principal, he completed his secondary education at the Argovian cantonal school (a gymnasium) in Aarau, Switzerland, graduating in 1896.[32] While lodging in Aarau with the family of Jost Winteler, he fell in love with Winteler's daughter, Marie. (His sister, Maja, later married Winteler's son Paul.[33])

Einstein's matriculation certificate at the age of 17. The heading translates as "The Education Committee of the Canton of Aargau". His scores were German 5, French 3, Italian 5, History 6, Geography 4, Algebra 6, Geometry 6, Descriptive Geometry 6, Physics 6, Chemistry 5, Natural History 5, Art Drawing 4, Technical Drawing 4. 6 = very good, 5 = good, 4 = sufficient, 3 = insufficient, 2 = poor, 1 = very poor.
Einstein's Matura certificate from canton Aargau, 1896[note 2]

In January 1896, with his father's approval, Einstein renounced his citizenship of the German Kingdom of Württemberg in order to avoid conscription into military service.[34] The Matura (graduation for the successful completion of higher secondary schooling), awarded to him in September 1896, acknowledged him to have performed well across most of the curriculum, allotting him a top grade of 6 for history, physics, algebra, geometry, and descriptive geometry.[35] At seventeen, he enrolled in the four-year mathematics and physics teaching diploma program at the federal polytechnic school. He befriended fellow student Marcel Grossmann, who would help him there to get by despite his loose study habits, and later to mathematically underpin his revolutionary insights into physics. Marie Winteler, a year older than him, took up a teaching post in Olsberg, Switzerland.[33]

The five other polytechnic school freshmen following the same course as Einstein included just one woman, a twenty year old Serbian, Mileva Marić. Over the next few years, the pair spent many hours discussing their shared interests and learning about topics in physics that the polytechnic school's lectures did not cover. In his letters to Marić, Einstein confessed that exploring science with her by his side was much more enjoyable than reading a textbook in solitude. Eventually the two students became not only friends but also lovers.[36]

Historians of physics are divided on the question of the extent to which Marić contributed to the insights of Einstein's annus mirabilis publications. There is at least some evidence that he was influenced by her scientific ideas,[36][37][38] but there are scholars who doubt whether her impact on his thought was of any great significance at all.[39][40][41][42]

Marriages, relationships and children

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Albert Einstein and Mileva Marić Einstein, 1912

Correspondence between Einstein and Marić, discovered and published in 1987, revealed that in early 1902, while Marić was visiting her parents in Novi Sad, she gave birth to a daughter, Lieserl. When Marić returned to Switzerland it was without the child, whose fate is uncertain. A letter of Einstein's that he wrote in September 1903 suggests that the girl was either given up for adoption or died of scarlet fever in infancy.[43][44]

Einstein and Marić married in January 1903. In May 1904, their son Hans Albert was born in Bern, Switzerland. Their son Eduard was born in Zurich in July 1910. In letters that Einstein wrote to Marie Winteler in the months before Eduard's arrival, he described his love for his wife as "misguided" and mourned the "missed life" that he imagined he would have enjoyed if he had married Winteler instead: "I think of you in heartfelt love every spare minute and am so unhappy as only a man can be."[45]

Einstein, looking relaxed and holding a pipe, stands next to a smiling, well-dressed Elsa who is wearing a fancy hat and fur wrap. She is looking at him.
Albert and Elsa Einstein arriving in New York, 1921

In 1912, Einstein entered into a relationship with Elsa Löwenthal, who was both his first cousin on his mother's side and his second cousin on his father's.[46][47][48] When Marić learned of his infidelity soon after moving to Berlin with him in April 1914, she returned to Zurich, taking Hans Albert and Eduard with her.[36] Einstein and Marić were granted a divorce on 14 February 1919 on the grounds of having lived apart for five years.[49][50] As part of the divorce settlement, Einstein agreed that if he were to win a Nobel Prize, he would give the money that he received to Marić; he won the prize two years later.[51]

Einstein married Löwenthal in 1919.[52][53] In 1923, he began a relationship with a secretary named Betty Neumann, the niece of his close friend Hans Mühsam.[54][55][56][57] Löwenthal nevertheless remained loyal to him, accompanying him when he emigrated to the United States in 1933. In 1935, she was diagnosed with heart and kidney problems. She died in December 1936.[58]

Albert and Elsa Einstein, 1930

A volume of Einstein's letters released by Hebrew University of Jerusalem in 2006[59] added some other women with whom he was romantically involved. They included Margarete Lebach (a married Austrian),[60] Estella Katzenellenbogen (the rich owner of a florist business), Toni Mendel (a wealthy Jewish widow) and Ethel Michanowski (a Berlin socialite), with whom he spent time and from whom he accepted gifts while married to Löwenthal.[61][62] After being widowed, Einstein was briefly in a relationship with Margarita Konenkova, thought by some to be a Russian spy; her husband, the Russian sculptor Sergei Konenkov, created the bronze bust of Einstein at the Institute for Advanced Study at Princeton.[63][64]

Following an episode of acute mental illness at about the age of twenty, Einstein's son Eduard was diagnosed with schizophrenia.[65] He spent the remainder of his life either in the care of his mother or in temporary confinement in an asylum. After her death, he was committed permanently to Burghölzli, the Psychiatric University Hospital in Zurich.[66]

Assistant at the Swiss Patent Office (1902–1909)

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Head and shoulders shot of a young, mustached man with dark, curly hair wearing a plaid suit and vest, striped shirt, and a dark tie.
Einstein at the Swiss patent office, 1904

Einstein graduated from the federal polytechnic school in 1900, duly certified as competent to teach mathematics and physics.[67] His successful acquisition of Swiss citizenship in February 1901[68] was not followed by the usual sequel of conscription; the Swiss authorities deemed him medically unfit for military service. He found that Swiss schools too appeared to have no use for him, failing to offer him a teaching position despite the almost two years that he spent applying for one. Eventually it was with the help of Marcel Grossmann's father that he secured a post in Bern at the Swiss Patent Office,[69][70] as an assistant examiner – level III.[71][72]

Patent applications that landed on Einstein's desk for his evaluation included ideas for a gravel sorter and an electric typewriter.[72] His employers were pleased enough with his work to make his position permanent in 1903, although they did not think that he should be promoted until he had "fully mastered machine technology".[73] It is conceivable that his labors at the patent office had a bearing on his development of his special theory of relativity. He arrived at his revolutionary ideas about space, time and light through thought experiments about the transmission of signals and the synchronization of clocks, matters which also figured in some of the inventions submitted to him for assessment.[10]

In 1902, Einstein and some friends whom he had met in Bern formed a group that held regular meetings to discuss science and philosophy. Their choice of a name for their club, the Olympia Academy, was an ironic comment upon its far from Olympian status. Sometimes they were joined by Marić, who limited her participation in their proceedings to careful listening.[74] The thinkers whose works they reflected upon included Henri Poincaré, Ernst Mach and David Hume, all of whom significantly influenced Einstein's own subsequent ideas and beliefs.[75]

First scientific papers (1900–1905)

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Cover image of the PhD dissertation of Albert Einstein
Einstein's 1905 dissertation, Eine neue Be­stimm­ung der Mol­e­kül­di­men­si­onen ("A new deter­mi­na­tion of mo­lec­u­lar di­men­sions")

Einstein's first paper, "Folgerungen aus den Capillaritätserscheinungen" ("Conclusions drawn from the phenomena of capillarity"), in which he proposed a model of intermolecular attraction that he afterwards disavowed as worthless, was published in the journal Annalen der Physik in 1901.[76][77] His 24-page doctoral dissertation also addressed a topic in molecular physics. Titled "Eine neue Bestimmung der Moleküldimensionen" ("A New Determination of Molecular Dimensions") and dedicated "Meinem Freunde Herr Dr. Marcel Grossmann gewidmet" (to his friend Marcel Grossman), it was completed on 30 April 1905[78] and approved by Professor Alfred Kleiner of the University of Zurich three months later. (Einstein was formally awarded his PhD on 15 January 1906.)[78][79][80] Four other pieces of work that Einstein completed in 1905—his famous papers on the photoelectric effect, Brownian motion, his special theory of relativity and the equivalence of mass and energy—have led to the year being celebrated as an annus mirabilis for physics akin to the miracle year of 1666 when Isaac Newton experienced his greatest epiphanies. The publications deeply impressed Einstein's contemporaries.[81]

Academic career in Europe (1908–1933)

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Einstein's sabbatical as a civil servant approached its end in 1908, when he secured a junior teaching position at the University of Bern. In 1909, a lecture on relativistic electrodynamics that he gave at the University of Zurich, much admired by Alfred Kleiner, led to Zurich's luring him away from Bern with a newly created associate professorship.[82] Promotion to a full professorship followed in April 1911, when he took up a chair at the German Charles-Ferdinand University in Prague,[83] a move which required him to become an Austrian citizen of the Austro-Hungarian Empire, which was not completed.[84] His time in Prague saw him producing eleven research papers.[85]

Einstein with colleagues at the ETH in Zurich, 1913

From 30 October to 3 November 1911, Einstein attended the first Solvay Conference on Physics.[86]

In July 1912, he returned to his alma mater, the ETH Zurich, to take up a chair in theoretical physics. His teaching activities there centered on thermodynamics and analytical mechanics, and his research interests included the molecular theory of heat, continuum mechanics and the development of a relativistic theory of gravitation. In his work on the latter topic, he was assisted by his friend Marcel Grossmann, whose knowledge of the kind of mathematics required was greater than his own.[87]

In the spring of 1913, two German visitors, Max Planck and Walther Nernst, called upon Einstein in Zurich in the hope of persuading him to relocate to Berlin.[88] They offered him membership of the Prussian Academy of Sciences, the directorship of the planned Kaiser Wilhelm Institute for Physics and a chair at the Humboldt University of Berlin that would allow him to pursue his research supported by a professorial salary but with no teaching duties to burden him.[47] Their invitation was all the more appealing to him because Berlin happened to be the home of his latest girlfriend, Elsa Löwenthal.[88] He duly joined the Academy on 24 July 1913,[89] and moved into an apartment in the Berlin district of Dahlem on 1 April 1914.[47] He was installed in his Humboldt University position shortly thereafter.[89]

Einstein with other physicists and chemists in Berlin, 1920

The outbreak of the First World War in July 1914 marked the beginning of Einstein's gradual estrangement from the nation of his birth. When the "Manifesto of the Ninety-Three" was published in October 1914—a document signed by a host of prominent German thinkers that justified Germany's belligerence—Einstein was one of the few German intellectuals to distance himself from it and sign the alternative, eirenic "Manifesto to the Europeans" instead.[90] However, this expression of his doubts about German policy did not prevent him from being elected to a two-year term as president of the German Physical Society in 1916.[91] When the Kaiser Wilhelm Institute for Physics opened its doors the following year—its foundation delayed because of the war—Einstein was appointed its first director, just as Planck and Nernst had promised.[92]

Einstein was elected a Foreign Member of the Royal Netherlands Academy of Arts and Sciences in 1920,[93] and a Foreign Member of the Royal Society in 1921. In 1922, he was awarded the 1921 Nobel Prize in Physics "for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect".[7] At this point some physicists still regarded the general theory of relativity skeptically, and the Nobel citation displayed a degree of doubt even about the work on photoelectricity that it acknowledged: it did not assent to Einstein's notion of the particulate nature of light, which only won over the entire scientific community when S. N. Bose derived the Planck spectrum in 1924. That same year, Einstein was elected an International Honorary Member of the American Academy of Arts and Sciences.[94] Britain's closest equivalent of the Nobel award, the Royal Society's Copley Medal, was not hung around Einstein's neck until 1925.[1] He was elected an International Member of the American Philosophical Society in 1930.[95]

Einstein resigned from the Prussian Academy in March 1933. His accomplishments in Berlin had included the completion of the general theory of relativity, proving the Einstein–de Haas effect, contributing to the quantum theory of radiation, and the development of Bose–Einstein statistics.[47]

Putting general relativity to the test (1919)

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The New York Times reported confirmation of the bending of light by gravitation after observations (made in Príncipe and Sobral) of the 29 May 1919 eclipse were presented to a joint meeting in London of the Royal Society and the Royal Astronomical Society on 6 November 1919.[96]

In 1907, Einstein reached a milestone on his long journey from his special theory of relativity to a new idea of gravitation with the formulation of his equivalence principle, which asserts that an observer in a box falling freely in a gravitational field would be unable to find any evidence that the field exists. In 1911, he used the principle to estimate the amount by which a ray of light from a distant star would be bent by the gravitational pull of the Sun as it passed close to the Sun's photosphere (that is, the Sun's apparent surface). He reworked his calculation in 1913, having now found a way to model gravitation with the Riemann curvature tensor of a non-Euclidean four-dimensional spacetime. By the fall of 1915, his reimagining of the mathematics of gravitation in terms of Riemannian geometry was complete, and he applied his new theory not just to the behavior of the Sun as a gravitational lens but also to another astronomical phenomenon, the precession of the perihelion of Mercury (a slow drift in the point in Mercury's elliptical orbit at which it approaches the Sun most closely).[47][97] A total eclipse of the Sun that took place on 29 May 1919 provided an opportunity to put his theory of gravitational lensing to the test, and observations performed by Sir Arthur Eddington yielded results that were consistent with his calculations. Eddington's work was reported at length in newspapers around the world. On 7 November 1919, for example, the leading British newspaper, The Times, printed a banner headline that read: "Revolution in Science – New Theory of the Universe – Newtonian Ideas Overthrown".[98]

Coming to terms with fame (1921–1923)

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Einstein's official portrait after receiving the 1921 Nobel Prize for Physics

With Eddington's eclipse observations widely reported not just in academic journals but by the popular press as well, Einstein became "perhaps the world's first celebrity scientist", a genius who had shattered a paradigm that had been basic to physicists' understanding of the universe since the seventeenth century.[99]

Einstein began his new life as an intellectual icon in America, where he arrived on 2 April 1921. He was welcomed to New York City by Mayor John Francis Hylan, and then spent three weeks giving lectures and attending receptions.[100] He spoke several times at Columbia University and Princeton, and in Washington, he visited the White House with representatives of the National Academy of Sciences. He returned to Europe via London, where he was the guest of the philosopher and statesman Viscount Haldane. He used his time in the British capital to meet several people prominent in British scientific, political or intellectual life, and to deliver a lecture at King's College.[101][102] In July 1921, he published an essay, "My First Impression of the U.S.A.", in which he sought to sketch the American character, much as had Alexis de Tocqueville in Democracy in America (1835).[103] He wrote of his transatlantic hosts in highly approving terms: "What strikes a visitor is the joyous, positive attitude to life ... The American is friendly, self-confident, optimistic, and without envy."[104]

In 1922, Einstein's travels were to the old world rather than the new. He devoted six months to a tour of Asia that saw him speaking in Japan, Singapore and Sri Lanka (then known as Ceylon). After his first public lecture in Tokyo, he met Emperor Yoshihito and his wife at the Imperial Palace, with thousands of spectators thronging the streets in the hope of catching a glimpse of him. (In a letter to his sons, he wrote that Japanese people seemed to him to be generally modest, intelligent and considerate, and to have a true appreciation of art.[105] But his picture of them in his diary was less flattering: "[the] intellectual needs of this nation seem to be weaker than their artistic ones – natural disposition?" His journal also contains views of China and India which were uncomplimentary. Of Chinese people, he wrote that "even the children are spiritless and look obtuse... It would be a pity if these Chinese supplant all other races. For the likes of us the mere thought is unspeakably dreary".[106][107]) He was greeted with even greater enthusiasm on the last leg of his tour, in which he spent twelve days in Mandatory Palestine, newly entrusted to British rule by the League of Nations in the aftermath of the First World War. Sir Herbert Samuel, the British High Commissioner, welcomed him with a degree of ceremony normally only accorded to a visiting head of state, including a cannon salute. One reception held in his honor was stormed by people determined to hear him speak: he told them that he was happy that Jews were beginning to be recognized as a force in the world.[105]

Einstein's decision to tour the eastern hemisphere in 1922 meant that he was unable to go to Stockholm in the December of that year to participate in the Nobel prize ceremony. His place at the traditional Nobel banquet was taken by a German diplomat, who gave a speech praising him not only as a physicist but also as a campaigner for peace.[108] A two-week visit to Spain that he undertook in 1923 saw him collecting another award, a membership of the Spanish Academy of Sciences signified by a diploma handed to him by King Alfonso XIII. (His Spanish trip also gave him a chance to meet a fellow Nobel laureate, the neuroanatomist Santiago Ramón y Cajal.)[109]

Serving the League of Nations (1922–1932)

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Einstein at a session of the International Committee on Intellectual Cooperation (League of Nations) of which he was a member from 1922 to 1932

From 1922 until 1932, with the exception of a few months in 1923 and 1924, Einstein was a member of the Geneva-based International Committee on Intellectual Cooperation of the League of Nations, a group set up by the League to encourage scientists, artists, scholars, teachers and other people engaged in the life of the mind to work more closely with their counterparts in other countries.[110][111] He was appointed as a German delegate rather than as a representative of Switzerland because of the machinations of two Catholic activists, Oskar Halecki and Giuseppe Motta. By persuading Secretary General Eric Drummond to deny Einstein the place on the committee reserved for a Swiss thinker, they created an opening for Gonzague de Reynold, who used his League of Nations position as a platform from which to promote traditional Catholic doctrine.[112] Einstein's former physics professor Hendrik Lorentz and the Polish chemist Marie Curie were also members of the committee.[113]

Touring South America (1925)

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In March and April 1925, Einstein and his wife visited South America, where they spent about a week in Brazil, a week in Uruguay and a month in Argentina.[114] Their tour was suggested by Jorge Duclout (1856–1927) and Mauricio Nirenstein (1877–1935)[115] with the support of several Argentine scholars, including Julio Rey Pastor, Jakob Laub, and Leopoldo Lugones. and was financed primarily by the Council of the University of Buenos Aires and the Asociación Hebraica Argentina (Argentine Hebraic Association) with a smaller contribution from the Argentine-Germanic Cultural Institution.[116]

Touring the US (1930–1931)

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Einstein in Pasadena, California, 1931

In December 1930, Einstein began another significant sojourn in the United States, drawn back to the US by the offer of a two month research fellowship at the California Institute of Technology. Caltech supported him in his wish that he should not be exposed to quite as much attention from the media as he had experienced when visiting the US in 1921, and he therefore declined all the invitations to receive prizes or make speeches that his admirers poured down upon him. But he remained willing to allow his fans at least some of the time with him that they requested.[117]

After arriving in New York City, Einstein was taken to various places and events, including Chinatown, a lunch with the editors of The New York Times, and a performance of Carmen at the Metropolitan Opera, where he was cheered by the audience on his arrival. During the days following, he was given the keys to the city by Mayor Jimmy Walker and met Nicholas Murray Butler, the president of Columbia University, who described Einstein as "the ruling monarch of the mind".[118] Harry Emerson Fosdick, pastor at New York's Riverside Church, gave Einstein a tour of the church and showed him a full-size statue that the church made of Einstein, standing at the entrance.[118] Also during his stay in New York, he joined a crowd of 15,000 people at Madison Square Garden during a Hanukkah celebration.[118]

Einstein with Charlie Chaplin at the Hollywood premiere of Chaplin's City Lights, January 1931

Einstein next traveled to California, where he met Caltech president and Nobel laureate Robert A. Millikan. His friendship with Millikan was "awkward", as Millikan "had a penchant for patriotic militarism", where Einstein was a pronounced pacifist.[119] During an address to Caltech's students, Einstein noted that science was often inclined to do more harm than good.[120]

This aversion to war also led Einstein to befriend author Upton Sinclair and film star Charlie Chaplin, both noted for their pacifism. Carl Laemmle, head of Universal Studios, gave Einstein a tour of his studio and introduced him to Chaplin. They had an instant rapport, with Chaplin inviting Einstein and his wife, Elsa, to his home for dinner. Chaplin said Einstein's outward persona, calm and gentle, seemed to conceal a "highly emotional temperament", from which came his "extraordinary intellectual energy".[121]

Chaplin's film City Lights was to premiere a few days later in Hollywood, and Chaplin invited Einstein and Elsa to join him as his special guests. Walter Isaacson, Einstein's biographer, described this as "one of the most memorable scenes in the new era of celebrity".[120] Chaplin visited Einstein at his home on a later trip to Berlin and recalled his "modest little flat" and the piano at which he had begun writing his theory. Chaplin speculated that it was "possibly used as kindling wood by the Nazis".[122] Einstein and Chaplin were cheered at the premiere of the film. Chaplin said to Einstein, "They cheer me because they understand me, and they cheer you because no one understands you."[120]

Emigration to the US (1933)

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Cartoon of Einstein, who has shed his "Pacifism" wings, standing next to a pillar labeled "World Peace". He is rolling up his sleeves and holding a sword labeled "Preparedness".
Cartoon of Einstein after shedding his "pacifism" wings (Charles R. Macauley, c. 1933)

In February 1933, while on a visit to the United States, Einstein knew he could not return to Germany with the rise to power of the Nazis under Germany's new chancellor, Adolf Hitler.[123][124]

While at American universities in early 1933, he undertook his third two-month visiting professorship at the California Institute of Technology in Pasadena. In February and March 1933, the Gestapo repeatedly raided his family's apartment in Berlin.[125] He and his wife Elsa returned to Europe in March, and during the trip, they learned that the German Reichstag had passed the Enabling Act on 23 March, transforming Hitler's government into a de facto legal dictatorship, and that they would not be able to proceed to Berlin. Later on, they heard that their cottage had been raided by the Nazis and Einstein's personal sailboat confiscated. Upon landing in Antwerp, Belgium on 28 March, Einstein immediately went to the German consulate and surrendered his passport, formally renouncing his German citizenship.[126] The Nazis later sold his boat and converted his cottage into a Hitler Youth camp.[127]

Refugee status

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Landing card for Einstein's 26 May 1933 arrival in Dover, England from Ostend, Belgium,[128] enroute to Oxford[129]

In April 1933, Einstein discovered that the new German government had passed laws barring Jews from holding any official positions, including teaching at universities.[130] Historian Gerald Holton describes how, with "virtually no audible protest being raised by their colleagues", thousands of Jewish scientists were suddenly forced to give up their university positions and their names were removed from the rolls of institutions where they were employed.[131]

A month later, Einstein's works were among those targeted by the German Student Union in the Nazi book burnings, with Nazi propaganda minister Joseph Goebbels proclaiming, "Jewish intellectualism is dead." One German magazine included him in a list of enemies of the German regime with the phrase, "not yet hanged", offering a $5,000 bounty on his head.[130][132] In a subsequent letter to physicist and friend Max Born, who had already emigrated from Germany to England, Einstein wrote, "... I must confess that the degree of their brutality and cowardice came as something of a surprise."[130] After moving to the US, he described the book burnings as a "spontaneous emotional outburst" by those who "shun popular enlightenment", and "more than anything else in the world, fear the influence of men of intellectual independence".[133]

Einstein was now without a permanent home, unsure where he would live and work, and equally worried about the fate of countless other scientists still in Germany. Aided by the Academic Assistance Council, founded in April 1933 by British Liberal politician William Beveridge to help academics escape Nazi persecution, Einstein was able to leave Germany.[134] He rented a house in De Haan, Belgium, where he lived for a few months. In late July 1933, he visited England for about six weeks at the invitation of the British Member of Parliament Commander Oliver Locker-Lampson, who had become friends with him in the preceding years.[128] Locker-Lampson invited him to stay near his Cromer home in a secluded wooden cabin on Roughton Heath in the Parish of Roughton, Norfolk. To protect Einstein, Locker-Lampson had two bodyguards watch over him; a photo of them carrying shotguns and guarding Einstein was published in the Daily Herald on 24 July 1933.[135][136]

Winston Churchill and Einstein at Chartwell House, 31 May 1933

Locker-Lampson took Einstein to meet Winston Churchill at his home, and later, Austen Chamberlain and former Prime Minister Lloyd George.[137] Einstein asked them to help bring Jewish scientists out of Germany. British historian Martin Gilbert notes that Churchill responded immediately, and sent his friend physicist Frederick Lindemann to Germany to seek out Jewish scientists and place them in British universities.[138] Churchill later observed that as a result of Germany having driven the Jews out, they had lowered their "technical standards" and put the Allies' technology ahead of theirs.[138]

Einstein later contacted leaders of other nations, including Turkey's Prime Minister, İsmet İnönü, to whom he wrote in September 1933, requesting placement of unemployed German-Jewish scientists. As a result of Einstein's letter, Jewish invitees to Turkey eventually totaled over "1,000 saved individuals".[139]

Locker-Lampson also submitted a bill to parliament to extend British citizenship to Einstein, during which period Einstein made a number of public appearances describing the crisis brewing in Europe.[140] In one of his speeches he denounced Germany's treatment of Jews, while at the same time he introduced a bill promoting Jewish citizenship in Palestine, as they were being denied citizenship elsewhere.[141] In his speech he described Einstein as a "citizen of the world" who should be offered a temporary shelter in the UK.[note 3][142] Both bills failed, however, and Einstein then accepted an earlier offer from the Institute for Advanced Study, in Princeton, New Jersey, US, to become a resident scholar.[140]

Resident scholar at the Institute for Advanced Study

[edit]
Portrait of Einstein taken in 1935 at Princeton

On 3 October 1933, Einstein delivered a speech on the importance of academic freedom before a packed audience at the Royal Albert Hall in London, with The Times reporting he was wildly cheered throughout.[134] Four days later he returned to the US and took up a position at the Institute for Advanced Study,[140][143] noted for having become a refuge for scientists fleeing Nazi Germany.[144] At the time, most American universities, including Harvard, Princeton and Yale, had minimal or no Jewish faculty or students, as a result of their Jewish quotas, which lasted until the late 1940s.[144]

Einstein was still undecided about his future. He had offers from several European universities, including Christ Church, Oxford, where he stayed for three short periods between May 1931 and June 1933[129] and was offered a five-year research fellowship (called a "studentship" at Christ Church),[145][146] but in 1935, he arrived at the decision to remain permanently in the United States and apply for citizenship.[140][147]

Einstein's affiliation with the Institute for Advanced Study would last until his death in 1955.[148] He was one of the four first selected (along with John von Neumann, Kurt Gödel and Hermann Weyl[149]) at the new Institute. He soon developed a close friendship with Gödel; the two would take long walks together discussing their work. Bruria Kaufman, his assistant, later became a physicist. During this period, Einstein tried to develop a unified field theory and to refute the accepted interpretation of quantum physics, both unsuccessfully. He lived in Princeton at his home from 1935 onwards. The Albert Einstein House was made a National Historic Landmark in 1976.

World War II and the Manhattan Project

[edit]
Facsimile of the Einstein–Szilard letter

In 1939, a group of Hungarian scientists that included émigré physicist Leó Szilárd attempted to alert Washington, D.C. to ongoing Nazi atomic bomb research. The group's warnings were discounted. Einstein and Szilárd, along with other refugees such as Edward Teller and Eugene Wigner, "regarded it as their responsibility to alert Americans to the possibility that German scientists might win the race to build an atomic bomb, and to warn that Hitler would be more than willing to resort to such a weapon."[150][151] To make certain the US was aware of the danger, in July 1939, a few months before the beginning of World War II in Europe, Szilárd and Wigner visited Einstein to explain the possibility of atomic bombs, which Einstein, a pacifist, said he had never considered.[152] He was asked to lend his support by writing a letter, with Szilárd, to President Franklin D. Roosevelt, recommending the US pay attention and engage in its own nuclear weapons research.

The letter is believed to be "arguably the key stimulus for the U.S. adoption of serious investigations into nuclear weapons on the eve of the U.S. entry into World War II".[153] In addition to the letter, Einstein used his connections with the Belgian royal family[154] and the Belgian queen mother to get access with a personal envoy to the White House's Oval Office. Some say that as a result of Einstein's letter and his meetings with Roosevelt, the US entered the "race" to develop the bomb, drawing on its "immense material, financial, and scientific resources" to initiate the Manhattan Project.

For Einstein, "war was a disease ... [and] he called for resistance to war." By signing the letter to Roosevelt, some argue he went against his pacifist principles.[155] In 1954, a year before his death, Einstein said to his old friend, Linus Pauling, "I made one great mistake in my life—when I signed the letter to President Roosevelt recommending that atom bombs be made; but there was some justification—the danger that the Germans would make them ..."[156] In 1955, Einstein and ten other intellectuals and scientists, including British philosopher Bertrand Russell, signed a manifesto highlighting the danger of nuclear weapons.[157] In 1960 Einstein was included posthumously as a charter member of the World Academy of Art and Science (WAAS),[158] an organization founded by distinguished scientists and intellectuals who committed themselves to the responsible and ethical advances of science, particularly in light of the development of nuclear weapons.

US citizenship

[edit]
Einstein accepting a US citizenship certificate from judge Phillip Forman in 1940

Einstein became an American citizen in 1940. Not long after settling into his career at the Institute for Advanced Study in Princeton, New Jersey, he expressed his appreciation of the meritocracy in American culture compared to Europe. He recognized the "right of individuals to say and think what they pleased" without social barriers. As a result, individuals were encouraged, he said, to be more creative, a trait he valued from his early education.[159]

Einstein joined the National Association for the Advancement of Colored People (NAACP) in Princeton, where he campaigned for the civil rights of African Americans. He considered racism America's "worst disease",[132][160] seeing it as "handed down from one generation to the next".[161] As part of his involvement, he corresponded with civil rights activist W. E. B. Du Bois and was prepared to testify on his behalf during his trial as an alleged foreign agent in 1951.[162] When Einstein offered to be a character witness for Du Bois, the judge decided to drop the case.[163]

In 1946, Einstein visited Lincoln University in Pennsylvania, a historically black college, where he was awarded an honorary degree. Lincoln was the first university in the United States to grant college degrees to African Americans; alumni include Langston Hughes and Thurgood Marshall. Einstein gave a speech about racism in America, adding, "I do not intend to be quiet about it."[164] A resident of Princeton recalls that Einstein had once paid the college tuition for a black student.[163] Einstein has said, "Being a Jew myself, perhaps I can understand and empathize with how black people feel as victims of discrimination".[160] Isaacson writes that "When Marian Anderson, the black contralto, came to Princeton for a concert in 1937, the Nassau Inn refused her a room. So Einstein invited her to stay at his house on Main Street, in what was a deeply personal as well as symbolic gesture ... Whenever she returned to Princeton, she stayed with Einstein, her last visit coming just two months before he died."[165]

Personal views

[edit]

Political views

[edit]
Casual group shot of four men and two women standing on a brick pavement.
Albert Einstein and Elsa Einstein arriving in New York in 1921. Accompanying them are Zionist leaders Chaim Weizmann (future president of Israel), Weizmann's wife Vera Weizmann, Menahem Ussishkin, and Ben-Zion Mossinson.

In 1918, Einstein was one of the signatories of the founding proclamation of the German Democratic Party, a liberal party.[166][167] Later in his life, Einstein's political view was in favor of socialism and critical of capitalism, which he detailed in his essays such as "Why Socialism?".[168][169] His opinions on the Bolsheviks also changed with time. In 1925, he criticized them for not having a "well-regulated system of government" and called their rule a "regime of terror and a tragedy in human history". He later adopted a more moderated view, criticizing their methods but praising them, which is shown by his 1929 remark on Vladimir Lenin:

In Lenin I honor a man, who in total sacrifice of his own person has committed his entire energy to realizing social justice. I do not find his methods advisable. One thing is certain, however: men like him are the guardians and renewers of mankind's conscience.[170]

Einstein offered and was called on to give judgments and opinions on matters often unrelated to theoretical physics or mathematics.[140] He strongly advocated the idea of a democratic global government that would check the power of nation-states in the framework of a world federation.[171] He wrote "I advocate world government because I am convinced that there is no other possible way of eliminating the most terrible danger in which man has ever found himself."[172] The FBI created a secret dossier on Einstein in 1932; by the time of his death, it was 1,427 pages long.[173]

Einstein was deeply impressed by Mahatma Gandhi, with whom he corresponded. He described Gandhi as "a role model for the generations to come".[174] The initial connection was established on 27 September 1931, when Wilfrid Israel took his Indian guest V. A. Sundaram to meet his friend Einstein at his summer home in the town of Caputh. Sundaram was Gandhi's disciple and special envoy, whom Wilfrid Israel met while visiting India and visiting the Indian leader's home in 1925. During the visit, Einstein wrote a short letter to Gandhi that was delivered to him through his envoy, and Gandhi responded quickly with his own letter. Although in the end Einstein and Gandhi were unable to meet as they had hoped, the direct connection between them was established through Wilfrid Israel.[175]

Relationship with Zionism

[edit]

Einstein was a figurehead leader in the establishment of the Hebrew University of Jerusalem,[176] which opened in 1925.[177] Earlier, in 1921, he was asked by the biochemist and president of the World Zionist Organization, Chaim Weizmann, to help raise funds for the planned university.[178] He made suggestions for the creation of an Institute of Agriculture, a Chemical Institute and an Institute of Microbiology in order to fight the various ongoing epidemics such as malaria, which he called an "evil" that was undermining a third of the country's development.[179] He also promoted the establishment of an Oriental Studies Institute, to include language courses given in both Hebrew and Arabic.[180]

Einstein was not a nationalist and opposed the creation of an independent Jewish state.[181] He felt that the waves of arriving Jews of the Aliyah could live alongside existing Arabs in Palestine. The state of Israel was established without his help in 1948; Einstein was limited to a marginal role in the Zionist movement.[182] Upon the death of Israeli president Weizmann in November 1952, Prime Minister David Ben-Gurion offered Einstein the largely ceremonial position of President of Israel at the urging of Ezriel Carlebach.[183][184] The offer was presented by Israel's ambassador in Washington, Abba Eban, who explained that the offer "embodies the deepest respect which the Jewish people can repose in any of its sons". Einstein wrote that he was "deeply moved", but "at once saddened and ashamed" that he could not accept it.[185] Einstein did not want the office, and Israel did not want him to accept, but felt obliged to make the offer. Yitzhak Navon, Ben-Gurion's political secretary, and later president, reports Ben-Gurion as saying "Tell me what to do if he says yes! I've had to offer the post to him because it's impossible not to. But if he accepts, we are in for trouble."[186]

Religious and philosophical views

[edit]
Opening of Einstein's speech (11 April 1943) for the United Jewish Appeal (recording by Radio Universidad Nacional de La Plata, Argentina)
"Ladies (coughs) and gentlemen, our age is proud of the progress it has made in man's intellectual development. The search and striving for truth and knowledge is one of the highest of man's qualities ..."

Per Lee Smolin, "I believe what allowed Einstein to achieve so much was primarily a moral quality. He simply cared far more than most of his colleagues that the laws of physics have to explain everything in nature coherently and consistently."[187] Einstein expounded his spiritual outlook in a wide array of writings and interviews.[188] He said he had sympathy for the impersonal pantheistic God of Baruch Spinoza's philosophy.[189] He did not believe in a personal god who concerns himself with fates and actions of human beings, a view which he described as naïve.[190] He clarified, however, that "I am not an atheist",[191] preferring to call himself an agnostic,[192][193] or a "deeply religious nonbeliever".[190] He wrote that "A spirit is manifest in the laws of the universe—a spirit vastly superior to that of man, and one in the face of which we with our modest powers must feel humble. In this way the pursuit of science leads to a religious feeling of a special sort."[194]

Einstein was primarily affiliated with non-religious humanist and Ethical Culture groups in both the UK and US. He served on the advisory board of the First Humanist Society of New York,[195] and was an honorary associate of the Rationalist Association, which publishes New Humanist in Britain. For the 75th anniversary of the New York Society for Ethical Culture, he stated that the idea of Ethical Culture embodied his personal conception of what is most valuable and enduring in religious idealism. He observed, "Without 'ethical culture' there is no salvation for humanity."[196]

In a German-language letter to philosopher Eric Gutkind, dated 3 January 1954, Einstein wrote:

The word God is for me nothing more than the expression and product of human weaknesses, the Bible a collection of honorable, but still primitive legends which are nevertheless pretty childish. No interpretation no matter how subtle can (for me) change this. ... For me the Jewish religion like all other religions is an incarnation of the most childish superstitions. And the Jewish people to whom I gladly belong and with whose mentality I have a deep affinity have no different quality for me than all other people. ... I cannot see anything 'chosen' about them.[197]

Einstein had been sympathetic toward vegetarianism for a long time. In a letter in 1930 to Hermann Huth, vice-president of the German Vegetarian Federation (Deutsche Vegetarier-Bund), he wrote:

Although I have been prevented by outward circumstances from observing a strictly vegetarian diet, I have long been an adherent to the cause in principle. Besides agreeing with the aims of vegetarianism for aesthetic and moral reasons, it is my view that a vegetarian manner of living by its purely physical effect on the human temperament would most beneficially influence the lot of mankind.[198]

He became a vegetarian himself only during the last part of his life. In March 1954 he wrote in a letter: "So I am living without fats, without meat, without fish, but am feeling quite well this way. It almost seems to me that man was not born to be a carnivore."[199]

Love of music

[edit]
Einstein playing the violin, 1927

Einstein developed an appreciation for music at an early age. In his late journals he wrote:

If I were not a physicist, I would probably be a musician. I often think in music. I live my daydreams in music. I see my life in terms of music ... I get most joy in life out of music.[200][201]

His mother played the piano reasonably well and wanted her son to learn the violin, not only to instill in him a love of music but also to help him assimilate into German culture. According to conductor Leon Botstein, Einstein began playing when he was 5. However, he did not enjoy it at that age.[202]

When he turned 13, he discovered Mozart's violin sonatas, whereupon he became enamored of Mozart's compositions and studied music more willingly. Einstein taught himself to play without "ever practicing systematically". He said that "love is a better teacher than a sense of duty".[202] At the age of 17, he was heard by a school examiner in Aarau while playing Beethoven's violin sonatas. The examiner stated afterward that his playing was "remarkable and revealing of 'great insight'". What struck the examiner, writes Botstein, was that Einstein "displayed a deep love of the music, a quality that was and remains in short supply. Music possessed an unusual meaning for this student."[202]

Music took on a pivotal and permanent role in Einstein's life from that period on. Although the idea of becoming a professional musician himself was not on his mind at any time, among those with whom Einstein played chamber music were a few professionals, including Kurt Appelbaum, and he performed for private audiences and friends. Chamber music had also become a regular part of his social life while living in Bern, Zurich, and Berlin, where he played with Max Planck and his son, among others. He is sometimes erroneously credited as the editor of the 1937 edition of the Köchel catalog of Mozart's work; that edition was prepared by Alfred Einstein, who may have been a distant relation.[203][204] Mozart was a special favorite; he said that "Mozart's music is so pure it seems to have been ever-present in the universe." However, he preferred Bach to Beethoven, once saying: "Give me Bach, rather, and then more Bach."[205]

In 1931, while engaged in research at the California Institute of Technology, he visited the Zoellner family conservatory in Los Angeles, where he played some of Beethoven and Mozart's works with members of the Zoellner Quartet.[206][207] Near the end of his life, when the young Juilliard Quartet visited him in Princeton, he played his violin with them, and the quartet was "impressed by Einstein's level of coordination and intonation".[202]

Death

[edit]

On 17 April 1955, Einstein experienced internal bleeding caused by the rupture of an abdominal aortic aneurysm, which had previously been reinforced surgically by Rudolph Nissen in 1948.[208] He took the draft of a speech he was preparing for a television appearance commemorating the state of Israel's seventh anniversary with him to the hospital, but he did not live to complete it.[209]

Einstein refused surgery, saying, "I want to go when I want. It is tasteless to prolong life artificially. I have done my share; it is time to go. I will do it elegantly."[210] He died in the Princeton Hospital early the next morning at the age of 76, having continued to work until near the end.[211]

During the autopsy, the pathologist Thomas Stoltz Harvey removed Einstein's brain for preservation without the permission of his family, in the hope that the neuroscience of the future would be able to discover what made Einstein so intelligent.[212] Einstein's remains were cremated in Trenton, New Jersey,[213] and his ashes were scattered at an undisclosed location.[214][215]

In a memorial lecture delivered on 13 December 1965 at UNESCO headquarters, nuclear physicist J. Robert Oppenheimer summarized his impression of Einstein as a person: "He was almost wholly without sophistication and wholly without worldliness ... There was always with him a wonderful purity at once childlike and profoundly stubborn."[216]

Einstein bequeathed his personal archives, library, and intellectual assets to the Hebrew University of Jerusalem in Israel.[217]

Scientific career

[edit]

Throughout his life, Einstein published hundreds of books and articles.[15][218] He published more than 300 scientific papers and 150 non-scientific ones.[11][218] On 5 December 2014, universities and archives announced the release of Einstein's papers, comprising more than 30,000 unique documents.[219][220] In addition to the work he did by himself, he also collaborated with other scientists on additional projects, including the Bose–Einstein statistics, the Einstein refrigerator and others.[221][222]

Statistical mechanics

[edit]

Thermodynamic fluctuations and statistical physics

[edit]

Einstein's first paper,[76][223] submitted in 1900 to Annalen der Physik, was on capillary attraction. It was published in 1901 with the title "Folgerungen aus den Capillaritätserscheinungen", which translates as "Conclusions from the capillarity phenomena". Two papers he published in 1902–1903 (thermodynamics) attempted to interpret atomic phenomena from a statistical point of view. These papers were the foundation for the 1905 paper on Brownian motion, which showed that Brownian movement can be construed as firm evidence that molecules exist. His research in 1903 and 1904 was mainly concerned with the effect of finite atomic size on diffusion phenomena.[223]

Theory of critical opalescence

[edit]

Einstein returned to the problem of thermodynamic fluctuations, giving a treatment of the density variations in a fluid at its critical point. Ordinarily the density fluctuations are controlled by the second derivative of the free energy with respect to the density. At the critical point, this derivative is zero, leading to large fluctuations. The effect of density fluctuations is that light of all wavelengths is scattered, making the fluid look milky white. Einstein relates this to Rayleigh scattering, which is what happens when the fluctuation size is much smaller than the wavelength, and which explains why the sky is blue.[224] Einstein quantitatively derived critical opalescence from a treatment of density fluctuations, and demonstrated how both the effect and Rayleigh scattering originate from the atomistic constitution of matter.

1905 – Annus Mirabilis papers

[edit]

The Annus Mirabilis papers are four articles pertaining to the photoelectric effect (which gave rise to quantum theory), Brownian motion, the special theory of relativity, and E = mc2 that Einstein published in the Annalen der Physik scientific journal in 1905. These four works contributed substantially to the foundation of modern physics and changed views on space, time, and matter. The four papers are:

Title (translated) Area of focus Received Published Significance
"On a Heuristic Viewpoint Concerning the Production and Transformation of Light"[225] Photoelectric effect 18 March 9 June Resolved an unsolved puzzle by suggesting that energy is exchanged only in discrete amounts (quanta).[226] This idea was pivotal to the early development of quantum theory.[227]
"On the Motion of Small Particles Suspended in a Stationary Liquid, as Required by the Molecular Kinetic Theory of Heat"[228] Brownian motion 11 May 18 July Explained empirical evidence for the atomic theory, supporting the application of statistical physics.
"On the Electrodynamics of Moving Bodies"[229] Special relativity 30 June 26 September Reconciled Maxwell's equations for electricity and magnetism with the laws of mechanics by introducing changes to mechanics, resulting from analysis based on the independence of the speed of light from the motion of the observer.[230] Discredited the concept of a "luminiferous ether".[231]
"Does the Inertia of a Body Depend Upon Its Energy Content?"[232] Matter–energy equivalence 27 September 21 November Equivalence of matter and energy, E = mc2, the existence of "rest energy", and the basis of nuclear energy.

Special relativity

[edit]

Einstein's "Zur Elektrodynamik bewegter Körper"[229] ("On the Electrodynamics of Moving Bodies") was received on 30 June 1905 and published 26 September of that same year. It reconciled conflicts between Maxwell's equations (the laws of electricity and magnetism) and the laws of Newtonian mechanics by introducing changes to the laws of mechanics.[233] Observationally, the effects of these changes are most apparent at high speeds (where objects are moving at speeds close to the speed of light). The theory developed in this paper later became known as Einstein's special theory of relativity.

This paper predicted that, when measured in the frame of a relatively moving observer, a clock carried by a moving body would appear to slow down, and the body itself would contract in its direction of motion. This paper also argued that the idea of a luminiferous aether—one of the leading theoretical entities in physics at the time—was superfluous.[note 4]

In his paper on mass–energy equivalence, Einstein produced E = mc2 as a consequence of his special relativity equations.[234] Einstein's 1905 work on relativity remained controversial for many years, but was accepted by leading physicists, starting with Max Planck.[note 5][235]

Einstein originally framed special relativity in terms of kinematics (the study of moving bodies). In 1908, Hermann Minkowski reinterpreted special relativity in geometric terms as a theory of spacetime. Einstein adopted Minkowski's formalism in his 1915 general theory of relativity.[236]

General relativity

[edit]

General relativity and the equivalence principle

[edit]
Black circle covering the sun, rays visible around it, in a dark sky.
Eddington's photo of a solar eclipse

General relativity (GR) is a theory of gravitation that was developed by Einstein between 1907 and 1915. According to it, the observed gravitational attraction between masses results from the warping of spacetime by those masses. General relativity has developed into an essential tool in modern astrophysics; it provides the foundation for the current understanding of black holes, regions of space where gravitational attraction is so strong that not even light can escape.[237]

As Einstein later said, the reason for the development of general relativity was that the preference of inertial motions within special relativity was unsatisfactory, while a theory which from the outset prefers no state of motion (even accelerated ones) should appear more satisfactory.[238] Consequently, in 1907 he published an article on acceleration under special relativity. In that article titled "On the Relativity Principle and the Conclusions Drawn from It", he argued that free fall is really inertial motion, and that for a free-falling observer the rules of special relativity must apply. This argument is called the equivalence principle. In the same article, Einstein also predicted the phenomena of gravitational time dilation, gravitational redshift and gravitational lensing.[239][240]

In 1911, Einstein published another article "On the Influence of Gravitation on the Propagation of Light" expanding on the 1907 article, in which he estimated the amount of deflection of light by massive bodies. Thus, the theoretical prediction of general relativity could for the first time be tested experimentally.[241]

Gravitational waves

[edit]

In 1916, Einstein predicted gravitational waves,[242][243] ripples in the curvature of spacetime which propagate as waves, traveling outward from the source, transporting energy as gravitational radiation. The existence of gravitational waves is possible under general relativity due to its Lorentz invariance which brings the concept of a finite speed of propagation of the physical interactions of gravity with it. By contrast, gravitational waves cannot exist in the Newtonian theory of gravitation, which postulates that the physical interactions of gravity propagate at infinite speed.

The first, indirect, detection of gravitational waves came in the 1970s through observation of a pair of closely orbiting neutron stars, PSR B1913+16.[244] The explanation for the decay in their orbital period was that they were emitting gravitational waves.[244][245] Einstein's prediction was confirmed on 11 February 2016, when researchers at LIGO published the first observation of gravitational waves,[246] detected on Earth on 14 September 2015, nearly one hundred years after the prediction.[244][247][248][249][250]

Hole argument and Entwurf theory

[edit]

While developing general relativity, Einstein became confused about the gauge invariance in the theory. He formulated an argument that led him to conclude that a general relativistic field theory is impossible. He gave up looking for fully generally covariant tensor equations and searched for equations that would be invariant under general linear transformations only.[251]

In June 1913, the Entwurf ('draft') theory was the result of these investigations. As its name suggests, it was a sketch of a theory, less elegant and more difficult than general relativity, with the equations of motion supplemented by additional gauge fixing conditions. After more than two years of intensive work, Einstein realized that the hole argument was mistaken[252] and abandoned the theory in November 1915.

Physical cosmology

[edit]
Robert A. Millikan, Georges Lemaître and Einstein at the California Institute of Technology in January 1933

In 1917, Einstein applied the general theory of relativity to the structure of the universe as a whole.[253] He discovered that the general field equations predicted a universe that was dynamic, either contracting or expanding. As observational evidence for a dynamic universe was lacking at the time, Einstein introduced a new term, the cosmological constant, into the field equations, in order to allow the theory to predict a static universe. The modified field equations predicted a static universe of closed curvature, in accordance with Einstein's understanding of Mach's principle in these years. This model became known as the Einstein World or Einstein's static universe.[254][255]

Following the discovery of the recession of the galaxies by Edwin Hubble in 1929, Einstein abandoned his static model of the universe, and proposed two dynamic models of the cosmos, the Friedmann–Einstein universe of 1931[256][257] and the Einstein–de Sitter universe of 1932.[258][259] In each of these models, Einstein discarded the cosmological constant, claiming that it was "in any case theoretically unsatisfactory".[256][257][260]

In many Einstein biographies, it is claimed that Einstein referred to the cosmological constant in later years as his "biggest blunder", based on a letter George Gamow claimed to have received from him. The astrophysicist Mario Livio has cast doubt on this claim.[261]

In late 2013, a team led by the Irish physicist Cormac O'Raifeartaigh discovered evidence that, shortly after learning of Hubble's observations of the recession of the galaxies, Einstein considered a steady-state model of the universe.[262][263] In a hitherto overlooked manuscript, apparently written in early 1931, Einstein explored a model of the expanding universe in which the density of matter remains constant due to a continuous creation of matter, a process that he associated with the cosmological constant.[264][265] As he stated in the paper, "In what follows, I would like to draw attention to a solution to equation (1) that can account for Hubbel's [sic] facts, and in which the density is constant over time [...] If one considers a physically bounded volume, particles of matter will be continually leaving it. For the density to remain constant, new particles of matter must be continually formed in the volume from space."

It thus appears that Einstein considered a steady-state model of the expanding universe many years before Hoyle, Bondi and Gold.[266][267] However, Einstein's steady-state model contained a fundamental flaw and he quickly abandoned the idea.[264][265][268]

Energy momentum pseudotensor

[edit]

General relativity includes a dynamical spacetime, so it is difficult to see how to identify the conserved energy and momentum. Noether's theorem allows these quantities to be determined from a Lagrangian with translation invariance, but general covariance makes translation invariance into something of a gauge symmetry. The energy and momentum derived within general relativity by Noether's prescriptions do not make a real tensor for this reason.[269]

Einstein argued that this is true for a fundamental reason: the gravitational field could be made to vanish by a choice of coordinates. He maintained that the non-covariant energy momentum pseudotensor was, in fact, the best description of the energy momentum distribution in a gravitational field. While the use of non-covariant objects like pseudotensors was criticized by Erwin Schrödinger and others, Einstein's approach has been echoed by physicists including Lev Landau and Evgeny Lifshitz.[270]

Wormholes

[edit]

In 1935, Einstein collaborated with Nathan Rosen to produce a model of a wormhole, often called Einstein–Rosen bridges.[271][272] His motivation was to model elementary particles with charge as a solution of gravitational field equations, in line with the program outlined in the paper "Do Gravitational Fields play an Important Role in the Constitution of the Elementary Particles?". These solutions cut and pasted Schwarzschild black holes to make a bridge between two patches. Because these solutions included spacetime curvature without the presence of a physical body, Einstein and Rosen suggested that they could provide the beginnings of a theory that avoided the notion of point particles. However, it was later found that Einstein–Rosen bridges are not stable.[273]

Einstein–Cartan theory

[edit]
Einstein, sitting at a table, looks up from the papers he is reading and into the camera.
Einstein at his office, University of Berlin, 1920

In order to incorporate spinning point particles into general relativity, the affine connection needed to be generalized to include an antisymmetric part, called the torsion. This modification was made by Einstein and Cartan in the 1920s.

Equations of motion

[edit]

In general relativity, gravitational force is reimagined as curvature of spacetime. A curved path like an orbit is not the result of a force deflecting a body from an ideal straight-line path, but rather the body's attempt to fall freely through a background that is itself curved by the presence of other masses. A remark by John Archibald Wheeler that has become proverbial among physicists summarizes the theory: "Spacetime tells matter how to move; matter tells spacetime how to curve."[274][275] The Einstein field equations cover the latter aspect of the theory, relating the curvature of spacetime to the distribution of matter and energy. The geodesic equation covers the former aspect, stating that freely falling bodies follow lines that are as straight as possible in a curved spacetime. Einstein regarded this as an "independent fundamental assumption" that had to be postulated in addition to the field equations in order to complete the theory. Believing this to be a shortcoming in how general relativity was originally presented, he wished to derive it from the field equations themselves. Since the equations of general relativity are non-linear, a lump of energy made out of pure gravitational fields, like a black hole, would move on a trajectory which is determined by the Einstein field equations themselves, not by a new law. Accordingly, Einstein proposed that the field equations would determine the path of a singular solution, like a black hole, to be a geodesic. Both physicists and philosophers have often repeated the assertion that the geodesic equation can be obtained from applying the field equations to the motion of a gravitational singularity, but this claim remains disputed.[276][277]

Old quantum theory

[edit]

Photons and energy quanta

[edit]
The photoelectric effect. Incoming photons on the left strike a metal plate (bottom), and eject electrons, depicted as flying off to the right.

In a 1905 paper,[225] Einstein postulated that light itself consists of localized particles (quanta). Einstein's light quanta were nearly universally rejected by all physicists, including Max Planck and Niels Bohr. This idea only became universally accepted in 1919, with Robert Millikan's detailed experiments on the photoelectric effect, and with the measurement of Compton scattering.

Einstein concluded that each wave of frequency f is associated with a collection of photons with energy hf each, where h is the Planck constant. He did not say much more, because he was not sure how the particles were related to the wave. But he did suggest that this idea would explain certain experimental results, notably the photoelectric effect.[225] Light quanta were dubbed photons by Gilbert N. Lewis in 1926.[278]

Quantized atomic vibrations

[edit]

In 1907, Einstein proposed a model of matter where each atom in a lattice structure is an independent harmonic oscillator. In the Einstein model, each atom oscillates independently—a series of equally spaced quantized states for each oscillator. Einstein was aware that getting the frequency of the actual oscillations would be difficult, but he nevertheless proposed this theory because it was a particularly clear demonstration that quantum mechanics could solve the specific heat problem in classical mechanics. Peter Debye refined this model.[279]

Bose–Einstein statistics

[edit]

In 1924, Einstein received a description of a statistical model from Indian physicist Satyendra Nath Bose, based on a counting method that assumed that light could be understood as a gas of indistinguishable particles. Einstein noted that Bose's statistics applied to some atoms as well as to the proposed light particles, and submitted his translation of Bose's paper to the Zeitschrift für Physik. Einstein also published his own articles describing the model and its implications, among them the Bose–Einstein condensate phenomenon that some particulates should appear at very low temperatures.[280] It was not until 1995 that the first such condensate was produced experimentally by Eric Allin Cornell and Carl Wieman using ultra-cooling equipment built at the NISTJILA laboratory at the University of Colorado at Boulder.[281] Bose–Einstein statistics are now used to describe the behaviors of any assembly of bosons. Einstein's sketches for this project may be seen in the Einstein Archive in the library of the Leiden University.[221]

Wave–particle duality

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Einstein in 1921, by Harris & Ewing studio

Although the patent office promoted Einstein to Technical Examiner Second Class in 1906, he had not given up on academia. In 1908, he became a Privatdozent at the University of Bern.[282] In "Über die Entwicklung unserer Anschauungen über das Wesen und die Konstitution der Strahlung" ("The Development of our Views on the Composition and Essence of Radiation"), on the quantization of light, and in an earlier 1909 paper, Einstein showed that Max Planck's energy quanta must have well-defined momenta and act in some respects as independent, point-like particles. This paper introduced the photon concept and inspired the notion of wave–particle duality in quantum mechanics. Einstein saw this wave–particle duality in radiation as concrete evidence for his conviction that physics needed a new, unified foundation.

Zero-point energy

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In a series of works completed from 1911 to 1913, Planck reformulated his 1900 quantum theory and introduced the idea of zero-point energy in his "second quantum theory". Soon, this idea attracted the attention of Einstein and his assistant Otto Stern. Assuming the energy of rotating diatomic molecules contains zero-point energy, they then compared the theoretical specific heat of hydrogen gas with the experimental data. The numbers matched nicely. However, after publishing the findings, they promptly withdrew their support, because they no longer had confidence in the correctness of the idea of zero-point energy.[283]

Stimulated emission

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In 1917, at the height of his work on relativity, Einstein published an article in Physikalische Zeitschrift that proposed the possibility of stimulated emission, the physical process that makes possible the maser and the laser.[284] This article showed that the statistics of absorption and emission of light would only be consistent with Planck's distribution law if the emission of light into a mode with n photons would be enhanced statistically compared to the emission of light into an empty mode. This paper was enormously influential in the later development of quantum mechanics, because it was the first paper to show that the statistics of atomic transitions had simple laws.[285]

Matter waves

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Einstein discovered Louis de Broglie's work and supported his ideas, which were received skeptically at first. In another major paper from this era, Einstein observed that de Broglie waves could explain the quantization rules of Bohr and Sommerfeld. This paper would inspire Schrödinger's work of 1926.[286][287]

Quantum mechanics

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Einstein's objections to quantum mechanics

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Newspaper headline on 4 May 1935

Einstein played a major role in developing quantum theory, beginning with his 1905 paper on the photoelectric effect. However, he became displeased with modern quantum mechanics as it had evolved after 1925, despite its acceptance by other physicists. He was skeptical that the randomness of quantum mechanics was fundamental rather than the result of determinism, stating that God "is not playing at dice".[288] Until the end of his life, he continued to maintain that quantum mechanics was incomplete.[289]

Bohr versus Einstein

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Two men sitting, looking relaxed. A dark-haired Bohr is talking while Einstein looks skeptical.
Einstein and Niels Bohr, 1925

The Bohr–Einstein debates were a series of public disputes about quantum mechanics between Einstein and Niels Bohr, who were two of its founders. Their debates are remembered because of their importance to the philosophy of science.[290][291][292] Their debates would influence later interpretations of quantum mechanics.

Einstein–Podolsky–Rosen paradox

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Einstein never fully accepted quantum mechanics. While he recognized that it made correct predictions, he believed a more fundamental description of nature must be possible. Over the years he presented multiple arguments to this effect, but the one he preferred most dated to a debate with Bohr in 1930. Einstein suggested a thought experiment in which two objects are allowed to interact and then moved apart a great distance from each other. The quantum-mechanical description of the two objects is a mathematical entity known as a wavefunction. If the wavefunction that describes the two objects before their interaction is given, then the Schrödinger equation provides the wavefunction that describes them after their interaction. But because of what would later be called quantum entanglement, measuring one object would lead to an instantaneous change of the wavefunction describing the other object, no matter how far away it is. Moreover, the choice of which measurement to perform upon the first object would affect what wavefunction could result for the second object. Einstein reasoned that no influence could propagate from the first object to the second instantaneously fast. Indeed, he argued, physics depends on being able to tell one thing apart from another, and such instantaneous influences would call that into question. Because the true "physical condition" of the second object could not be immediately altered by an action done to the first, Einstein concluded, the wavefunction could not be that true physical condition, only an incomplete description of it.[293][294]

A more famous version of this argument came in 1935, when Einstein published a paper with Boris Podolsky and Nathan Rosen that laid out what would become known as the EPR paradox.[295] In this thought experiment, two particles interact in such a way that the wavefunction describing them is entangled. Then, no matter how far the two particles were separated, a precise position measurement on one particle would imply the ability to predict, perfectly, the result of measuring the position of the other particle. Likewise, a precise momentum measurement of one particle would result in an equally precise prediction for of the momentum of the other particle, without needing to disturb the other particle in any way. They argued that no action taken on the first particle could instantaneously affect the other, since this would involve information being transmitted faster than light, which is forbidden by the theory of relativity. They invoked a principle, later known as the "EPR criterion of reality", positing that: "If, without in any way disturbing a system, we can predict with certainty (i.e., with probability equal to unity) the value of a physical quantity, then there exists an element of reality corresponding to that quantity." From this, they inferred that the second particle must have a definite value of both position and of momentum prior to either quantity being measured. But quantum mechanics considers these two observables incompatible and thus does not associate simultaneous values for both to any system. Einstein, Podolsky, and Rosen therefore concluded that quantum theory does not provide a complete description of reality.[296]

In 1964, John Stewart Bell carried the analysis of quantum entanglement much further. He deduced that if measurements are performed independently on the two separated particles of an entangled pair, then the assumption that the outcomes depend upon hidden variables within each half implies a mathematical constraint on how the outcomes on the two measurements are correlated. This constraint would later be called a Bell inequality. Bell then showed that quantum physics predicts correlations that violate this inequality. Consequently, the only way that hidden variables could explain the predictions of quantum physics is if they are "nonlocal", which is to say that somehow the two particles are able to interact instantaneously no matter how widely they ever become separated.[297][298] Bell argued that because an explanation of quantum phenomena in terms of hidden variables would require nonlocality, the EPR paradox "is resolved in the way which Einstein would have liked least".[299]

Despite this, and although Einstein personally found the argument in the EPR paper overly complicated,[293][294] that paper became among the most influential papers published in Physical Review. It is considered a centerpiece of the development of quantum information theory.[300]

Unified field theory

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Encouraged by his success with general relativity, Einstein sought an even more ambitious geometrical theory that would treat gravitation and electromagnetism as aspects of a single entity. In 1950, he described his unified field theory in a Scientific American article titled "On the Generalized Theory of Gravitation".[301] His attempt to find the most fundamental laws of nature won him praise but not success: a particularly conspicuous blemish of his model was that it did not accommodate the strong and weak nuclear forces, neither of which was well understood until many years after his death. Although most researchers now believe that Einstein's approach to unifying physics was mistaken, his goal of a theory of everything is one to which his successors still aspire.[302]

Other investigations

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Einstein conducted other investigations that were unsuccessful and abandoned. These pertain to force, superconductivity, and other research.

Collaboration with other scientists

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The 1927 Solvay Conference in Brussels, a gathering of the world's top physicists. Einstein is in the center.

In addition to longtime collaborators Leopold Infeld, Nathan Rosen, Peter Bergmann and others, Einstein also had some one-shot collaborations with various scientists.

Einstein–de Haas experiment

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In 1908, Owen Willans Richardson predicted that a change in the magnetic moment of a free body will cause this body to rotate. This effect is a consequence of the conservation of angular momentum and is strong enough to be observable in ferromagnetic materials.[303] Einstein and Wander Johannes de Haas published two papers in 1915 claiming the first experimental observation of the effect.[304][305] Measurements of this kind demonstrate that the phenomenon of magnetization is caused by the alignment (polarization) of the angular momenta of the electrons in the material along the axis of magnetization. These measurements also allow the separation of the two contributions to the magnetization: that which is associated with the spin and with the orbital motion of the electrons. The Einstein-de Haas experiment is the only experiment conceived, realized and published by Albert Einstein himself.

A complete original version of the Einstein-de Haas experimental equipment was donated by Geertruida de Haas-Lorentz, wife of de Haas and daughter of Lorentz, to the Ampère Museum in Lyon France in 1961 where it is currently on display. It was lost among the museum's holdings and was rediscovered in 2023.[306][307]

Einstein as an inventor

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In 1926, Einstein and his former student Leó Szilárd co-invented (and in 1930, patented) the Einstein refrigerator. This absorption refrigerator was then revolutionary for having no moving parts and using only heat as an input.[308] On 11 November 1930, U.S. patent 1,781,541 was awarded to Einstein and Leó Szilárd for the refrigerator. Their invention was not immediately put into commercial production, but the most promising of their patents were acquired by the Swedish company Electrolux.[note 6]

Einstein also invented an electromagnetic pump,[310] sound reproduction device,[311] and several other household devices.[312]

Legacy

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Non-scientific

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Left-right: Heinrich Goldschmidt, Einstein, Ole Colbjørnsen, Jørgen Vogt, and Ilse Einstein at a picnic in Oslo in 1920.

While traveling, Einstein wrote daily to his wife Elsa and adopted stepdaughters Margot and Ilse. The letters were included in the papers bequeathed to the Hebrew University of Jerusalem. Margot Einstein permitted the personal letters to be made available to the public, but requested that it not be done until twenty years after her death (she died in 1986[313]). Barbara Wolff, of the Hebrew University's Albert Einstein Archives, told the BBC that there are about 3,500 pages of private correspondence written between 1912 and 1955.[314]

In his final four years, Einstein was involved with the establishment of the Albert Einstein College of Medicine in New York City.[315]

In 1979, the Albert Einstein Memorial was unveiled outside the National Academy of Sciences building in Washington, D.C. for the Einstein centenary. It was sculpted by Robert Berks. Einstein can be seen holding a paper with three of his most important equations: for the photoelectric effect, general relativity and mass-energy equivalence.[316]

Einstein's right of publicity was litigated in 2015 in a federal district court in California. Although the court initially held that the right had expired,[317] that ruling was immediately appealed, and the decision was later vacated in its entirety. The underlying claims between the parties in that lawsuit were ultimately settled. The right is enforceable, and the Hebrew University of Jerusalem is the exclusive representative of that right.[318] Corbis, successor to The Roger Richman Agency, licenses the use of his name and associated imagery, as agent for the university.[319]

Mount Einstein in the Chugach Mountains of Alaska was named in 1955. Mount Einstein in New Zealand's Paparoa Range was named after him in 1970 by the Department of Scientific and Industrial Research.[320]

In 1999, Einstein was named Time's Person of the Century.[321]

Scientific

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In 1999, a survey of the top 100 physicists voted for Einstein as the "greatest physicist ever", while a parallel survey of rank-and-file physicists gave the top spot to Isaac Newton, with Einstein second.[322][323]

Physicist Lev Landau ranked physicists from 0 to 5 on a logarithmic scale of productivity and genius, with Newton and Einstein belonging in a "super league", with Newton receiving the highest ranking of 0, followed by Einstein with 0.5, while fathers of quantum mechanics such as Werner Heisenberg and Paul Dirac were ranked 1, with Landau himself a 2.[324]

Physicist Eugene Wigner noted that while John von Neumann had the quickest and most acute mind he ever knew, it was Einstein who had the more penetrating and original mind of the two, stating that:[325]

But Einstein's understanding was deeper than even Jancsi von Neumann's. His mind was both more penetrating and more original than von Neumann's. And that is a very remarkable statement. Einstein took an extraordinary pleasure in invention. Two of his greatest inventions are the Special and General Theories of Relativity; and for all of Jancsi's brilliance, he never produced anything so original. No modern physicist has.

The International Union of Pure and Applied Physics declared 2005 the "World Year of Physics", also known as "Einstein Year", in recognition of Einstein's "miracle year" in 1905.[326] It was also declared the "International Year of Physics" by the United Nations.[327]

[edit]
The famous image of Einstein taken by Arthur Sasse in 1951, sitting in a car on his 72nd birthday, having been asked to smile for the camera once again.

Einstein became one of the most famous scientific celebrities after the confirmation of his general theory of relativity in 1919.[328][329][330] Although most of the public had little understanding of his work, he was widely recognized and admired. In the period before World War II, The New Yorker published a vignette in their "The Talk of the Town" feature saying that Einstein was so well known in America that he would be stopped on the street by people wanting him to explain "that theory". Eventually he came to cope with unwanted enquirers by pretending to be someone else: "Pardon me, sorry! Always I am mistaken for Professor Einstein."[331]

Einstein has been the subject of or inspiration for many novels, films, plays, and works of music.[332] He is a favorite model for depictions of absent-minded professors; his expressive face and distinctive hairstyle have been widely copied and exaggerated. Time magazine's Frederic Golden wrote that Einstein was "a cartoonist's dream come true".[333] His intellectual achievements and originality made Einstein broadly synonymous with genius.[334]

Many popular quotations are often misattributed to him.[335][336]

Awards and honors

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Einstein received numerous awards and honors, and in 1922, he was awarded the 1921 Nobel Prize in Physics "for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect". None of the nominations in 1921 met the criteria set by Alfred Nobel, so the 1921 prize was carried forward and awarded to Einstein in 1922.[7]

Einsteinium, a synthetic chemical element, was named in his honor in 1955, a few months after his death.[337]

Publications

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Scientific

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Political

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See also

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Notes

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Albert Einstein (14 March 1879 – 18 April 1955) was a German-born theoretical physicist. He developed the theory of special relativity in 1905, establishing mass-energy equivalence through E = mc², and the general theory of relativity in 1915. His explanation of the photoelectric effect illuminated light's particle-like behavior, foundational to quantum mechanics, and earned him the 1921 Nobel Prize in Physics. Born to secular Ashkenazi Jewish parents in Ulm, Germany, Einstein fled Nazi persecution in 1933. He settled in the United States as a dual Swiss-American citizen and continued work on unified field theories at the Institute for Advanced Study in Princeton. He advocated pacifism and civil rights and supported Zionism mainly as a cultural and humanitarian project, while warning against narrow nationalism and urging Jewish–Arab cooperation, though his enduring influence stems primarily from transforming modern physics, with relativity theories essential for the accuracy of technologies such as GPS.[1]

Early Life and Education

Birth, Family, and Childhood

Albert Einstein was born on March 14, 1879, at 11:30 a.m. in Ulm, Kingdom of Württemberg, German Empire. He was the first child of Hermann Einstein and Pauline Koch, both secular Ashkenazi Jews.[2][3] Hermann, born August 30, 1847, in Bad Buchau, began as a featherbed salesman. He later partnered with his brother Jakob in electrochemical and electrical engineering, including gas and water supply systems and direct current equipment.[4][5][6] Pauline, born February 8, 1858, in Bad Cannstatt, played piano and mandolin. She came from a grain trading family and married Hermann in 1876 after he shifted the family business to technical work.[7][8] In June 1880, about 15 months after Einstein's birth, the family moved to Munich. There, Hermann and Jakob started an electrical engineering firm focused on lighting and dynamos to use new electrification technology.[2] Einstein's sister, Maria (Maja), was born in Munich on November 18, 1881, and became his close companion.[9] The middle-class family had a stable home, though Hermann's business later struggled against alternating current systems.[10] In Munich, young Einstein showed curiosity about nature. At age five, a pocket compass fascinated him with its unseen forces, sparking lifelong wonder.[5] At six, he began violin lessons from his mother, gaining a love for Mozart despite early resistance. He attended a local Catholic elementary school from age six, fitting into Bavarian society as a secular family. He had no major delays, though he spoke late until age three.[11] At eight, he started at Luitpold Gymnasium. He disliked its strict rote learning and discipline, which he said killed creativity. Instead, he studied Euclid's geometry and Kant's philosophy from family books.[3][12]

Education and Intellectual Formations

Portrait of Albert Einstein
Albert Einstein
Einstein began primary education at Munich's Petersschule in 1885, studying alongside Catholic religious instruction despite his Jewish background.[13] In 1888 he moved to the Luitpold Gymnasium, which he criticised for its rote memorisation and rigid teaching.[14] Outside school he taught himself algebra, Euclidean geometry, and calculus by age twelve, and developed an original proof of the Pythagorean theorem based on triangle similarity without formal instruction.[3] Family tutor Max Talmud introduced him to higher mathematics and philosophy, though Einstein quickly surpassed him. By fourteen he had mastered differential and integral calculus through self-study, and at sixteen wrote his first scientific essay — an unpublished work titled "On the Investigation of the State of the Ether in a Magnetic Field" — foreshadowing his later interests in light and relativity. In 1894, his family moved to Italy after business troubles. Einstein stayed in Munich to finish school but left after six months without a diploma due to the rigid system.[3] He joined them in Pavia and took the entrance exam for the Swiss Federal Polytechnic (ETH Zurich) in 1895. He passed science and math but failed languages and history, so he needed more preparation.[13] He attended the Kantonsschule in Aarau, Switzerland, a school that encouraged critical thinking and student independence under headmaster Jost Winteler. This suited his style and shaped his ideas on education.[14] He graduated in September 1896 with top marks (6 out of 6) in math, physics, and geometry but lower scores (like 3 in French) in languages.[3]
Profile portrait of Immanuel Kant
Immanuel Kant
In 1896, Einstein gave up German citizenship to avoid army service. At age 17, he entered ETH Zurich for a diploma in teaching physics and math.[14] There, he skipped many classes for self-study using textbooks, problems, thought experiments, and visual methods. He borrowed notes from friend Marcel Grossmann instead of taking his own.[13] He read philosophy, including Immanuel Kant's works on knowledge, space, time, and science methods.[15] He connected with professors like Hermann Minkowski and studied mechanics and electromagnetism deeply. His grades varied, and he graduated in 1900 as the only physics student to pass, without honors.[13] This time built his preference for intuitive, first-principles thinking over memorization, aiding his later work.[16]

Initial Career and Revolutionary Insights

Employment at the Swiss Patent Office

Portrait of young Albert Einstein
Albert Einstein around the time he began working at the Swiss Patent Office
After completing his studies at the Swiss Federal Polytechnic in 1900 and struggling to secure an academic position, Albert Einstein obtained employment at the Swiss Federal Patent Office in Bern through his university friend Marcel Grossmann, who alerted him to a vacancy.[17] He was appointed technical expert third class on June 23, 1902, initially provisional but soon permanent, with an annual salary of 3,500 Swiss francs that provided financial stability.[18][18]
Interior of the Swiss Patent Office in Bern
The Swiss Patent Office in Bern where Einstein worked as a technical expert
Einstein's duties centered on reviewing patent applications in mechanical and electromechanical fields, assessing novelty, feasibility, and patentability while drafting descriptions to protect intellectual property—tasks requiring precise logical analysis and skepticism toward unsubstantiated claims.[19][20] The role proved undemanding, typically completed in eight hours, leaving time for independent theoretical work.[21] On April 1, 1906, Einstein advanced to technical expert second class for his competence in handling complex submissions; his supervisor, Friedrich Haller, praised his quick grasp of technical problems, which Einstein said honed his critical faculties for physics.[21][22] He resigned effective October 15, 1909, to take a professorship at the University of Zurich, ending a period of stable routine that contrasted academic pressures and supported focused reflection amid practical scrutiny of inventions.[22] This environment fostered disciplined thought processes similar to deriving principles from observations, though direct causation is interpretive rather than proven.[23] Einstein produced seminal papers, including those of 1905, publishing over two dozen articles without job interference.[23]

Annus Mirabilis Papers (1905)

Albert Einstein in 1905
Albert Einstein in 1905, the year he published his four revolutionary papers
In 1905, Albert Einstein, a 26-year-old technical expert at the Swiss Patent Office in Bern without an academic position, published four groundbreaking papers in Annalen der Physik that transformed physics. These addressed the photoelectric effect, Brownian motion, special relativity, and mass-energy equivalence, yielding insights from first-principles analysis of experiments and theoretical issues.[24][25] The first, "Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt" (received March 18), proposed light as discrete quanta (later photons) with energy E=hνE = h\nu, where hh is Planck's constant and ν\nu is frequency. Extending Max Planck's quantum idea from blackbody radiation, it explained the photoelectric effect: a threshold frequency for electron emission regardless of intensity, with kinetic energy linear in frequency above threshold. This resolved classical wave theory's conflicts with experiments by Lenard and others, foundational for quantum mechanics despite initial skepticism. Einstein earned the 1921 Nobel Prize for this work.[26][27] The second, "Über die von der molekularkinetischen Theorie der Wärme geforderte Bewegung von in ruhenden Flüssigkeiten suspendierten Teilchen" (received May 11), derived Brownian motion theoretically via kinetic theory. Einstein found mean squared displacement x2=2Dt\langle x^2 \rangle = 2Dt, linking diffusion constant DD to temperature, viscosity, and radius per Stokes' law, offering evidence for atoms. Verified by Perrin in 1908–1909, it countered doubts from Ostwald and Mach.[28][25] The third, "Zur Elektrodynamik bewegter Körper" (received June 30), established special relativity. Einstein invoked the relativity principle (identical physics laws in inertial frames) and constant light speed cc in vacuum. Discarding the luminiferous ether, he derived Lorentz transformations, revealing time dilation, length contraction, and relativity of simultaneity—resolving Maxwell's electrodynamics and mechanics asymmetries. It unified space and time into spacetime, abolishing absolute motion.[25][29]
Page from Einstein's 1905 paper on mass-energy equivalence
Excerpt from Einstein's September 1905 paper 'Ist die Trägheit eines Körpers von seinem Energieinhalt abhängig?' deriving mass-energy equivalence
The fourth, "Ist die Trägheit eines Körpers von seinem Energieinhalt abhängig?" (received September 27, published November 21), derived E=mc2E = mc^2. Via a thought experiment of oppositely emitted light pulses, Einstein showed mass loss by L/c2L/c^2 (emitted energy LL), linking inertial mass to energy. This relativistic interchangeability proved crucial for nuclear physics.[30][25]

Theories of Relativity

Special Relativity Formulation

Historical page on electromagnetic theory of light with equations
Excerpt from a historical physics text discussing Maxwell's equations for electromagnetic waves
Einstein published special relativity in his 1905 paper "On the Electrodynamics of Moving Bodies," received by Annalen der Physik on June 30.[31] The theory resolved conflicts between Newtonian mechanics, which assumes absolute space and time, and Maxwell's equations for electromagnetism. These equations predict that light travels at constant speed c ≈ 3 × 10^8 m/s in vacuum, regardless of the source's motion, without an ether medium.[32] Einstein rejected the stationary luminiferous ether as unnecessary. He emphasized theoretical consistency over specific experiments, such as the 1887 Michelson-Morley experiment, which detected no ether.[32][33]
Albert Einstein standing in front of a chalkboard with diagrams
Albert Einstein beside a blackboard with mathematical drawings
Special relativity rests on two postulates. The first is the principle of relativity: the laws of physics take the same form in all inertial frames—reference systems that move at constant velocity relative to each other without acceleration. This extends Galileo's principle from mechanics to all physics, including electrodynamics.[32] The second postulate states that the speed of light in vacuum, c, is constant for all observers, regardless of the source's or observer's motion. This eliminates asymmetries in classical predictions, where relative motion would alter light speed.[32] Einstein derived these postulates from basic electrodynamic scenarios, such as moving conductors and magnets, without relying on ad hoc adjustments like length contractions in earlier Lorentz-FitzGerald theories.[32] From these postulates, Einstein derived the Lorentz transformations, which relate coordinates between inertial frames moving at constant velocity v along the x-axis. He assumed linearity based on spatial homogeneity and isotropy. Simultaneity is defined using light signals: events are simultaneous in a frame if light from their midpoint reaches observers there at the same time.[34][32] For frames S and S' (S' moving at v relative to S), the transformations are x' = γ(x - vt), t' = γ(t - vx/c²), y' = y, z' = z, where γ = 1 / √(1 - v²/c²) is the Lorentz factor.[32] The inverse transformations follow from reciprocity. These preserve the spacetime interval ds² = c²dt² - dx² - dy² - dz², defining the theory's causal structure.[34] The transformations imply relativity of simultaneity, time dilation (a moving clock's proper time τ slows: τ = t / γ), and length contraction (L = L₀ / γ along the motion direction). All derive directly from the postulates.[32] The theory combines space and time into Minkowski spacetime, later viewed geometrically. It includes relativistic kinematics: momentum p = γmv and total energy E = γmc², with rest energy E = mc².[32] Particle accelerator tests confirm time dilation accurately, validating predictions that challenge absolute time.[35]

General Relativity Development and Equivalence Principle

After formulating special relativity in 1905, Einstein saw that it covered only inertial frames and constant speeds. He needed to extend it to include acceleration and gravity, viewing them as effects of spacetime geometry.[36] In 1907, while at the Bern Patent Office, he had his key insight: the equivalence principle. This states that the effects of a uniform gravitational field match those of uniform acceleration in the opposite direction, making them locally indistinguishable.[37] Einstein called this idea—picturing a free-falling observer feeling no gravity—his "happiest thought."[38] The equivalence principle forms the basis of general relativity. It expands the relativity principle to all frames, even accelerated ones. Gravity thus emerges from the curvature of spacetime, the four-dimensional fabric combining space and time, rather than a distant force. Einstein used thought experiments to show this. For example, in a closed elevator accelerating upward at 9.8 m/s² in space, a person feels a downward force like Earth's gravity. A dropped object or light beam bends the same way. In free fall in gravity, local effects vanish, as tidal forces—stretches from uneven gravity—are small over short distances.[39] This requires describing spacetime with a metric, where freely falling paths, called geodesics (straight lines in curved space), replace Euclidean straight lines and Newtonian absolutes.[36] Einstein took eight years to complete the theory, facing math challenges. Special relativity used flat Minkowski spacetime, unfit for varying curvature.[38] In 1912, as a professor at ETH Zurich, he worked with classmate Marcel Grossmann. Grossmann introduced Riemannian geometry, which handles curved multidimensional spaces, and tensor calculus, tools for laws invariant under coordinate shifts.[40] Their 1913 paper sketched an "Entwurf" theory with a limited metric assuming absolute time. It predicted light bending by gravity but lacked full covariance, the property of holding under any coordinates.[36]
Handwritten manuscript page by Albert Einstein
Page from Einstein's 'Die Grundlage der allgemeinen Relativitätstheorie' (1916)
From 1914 in Berlin, Einstein dropped the Entwurf's limits. He refined a variational method to get field equations linking curvature to matter-energy.[40] He shared early versions with the Prussian Academy on November 4, 11, and 18, 1915. On November 25, he finalized the generally covariant Einstein field equations Gμν=8πGc4TμνG_{\mu\nu} = \frac{8\pi G}{c^4} T_{\mu\nu}. Here, GμνG_{\mu\nu} measures curvature using the Ricci tensor, and TμνT_{\mu\nu} represents the stress-energy tensor of matter and energy.[41] These equations fixed issues like Mercury's perihelion shift—43 arcseconds per century more than Newton's prediction—and made general relativity invariant under diffeomorphisms, rooted in the equivalence principle's causality.[42]

Predictions, Tests, and Cosmological Implications

General relativity made key predictions about gravity's effects, many confirmed by experiments. It explained Mercury's orbit precession—the wobble of its closest point to the Sun—at 43 arcseconds per century beyond Newtonian predictions. Einstein calculated this on November 18, 1915, and published it on November 25, 1915, matching the discrepancy observed since the 1850s.[43] The theory also predicted starlight deflection by 1.75 arcseconds when passing near the Sun, twice special relativity's value due to spacetime bending by gravity.[44] Teams led by Arthur Eddington on Príncipe and Andrew Crommelin in Sobral, Brazil, tested this during the May 29, 1919, solar eclipse. They measured about 1.6 arcseconds, matching general relativity within error margins. Results were announced on November 6, 1919.[45] Gravitational redshift, another prediction, states light loses energy climbing out of a gravity field, shifting to redder wavelengths. The 1959–1960 Pound–Rebka experiment at Harvard confirmed this with gamma rays over 22.5 meters in Earth's gravity. It detected a frequency shift of (2.56 ± 0.25) × 10⁻¹⁵, close to the predicted 2.5 × 10⁻¹⁵.[46]
Event Horizon Telescope images of black hole shadow testing general relativity
The black hole shadow in Messier 87 imaged by the Event Horizon Telescope in 2019, with comparisons showing agreement with general relativity predictions
Later tests confirmed predictions with high precision. Einstein predicted gravitational waves—ripples in spacetime from accelerating masses like orbiting stars—in 1916. LIGO detected them on September 14, 2015, from two black holes merging 1.3 billion light-years away. The signal matched theory within 1% deviation.[47] Black holes, where gravity traps light beyond an event horizon, gained visual proof in 2019. The Event Horizon Telescope imaged Messier 87's supermassive black hole shadow—a dark center ringed by light—with a size fitting predictions for a 6.5 billion solar mass rotating (Kerr) black hole.[48] In cosmology, general relativity described a dynamic universe. Einstein added a positive cosmological constant Λ in 1917 to allow a static cosmos, balancing gravity without expansion.[49] Alexander Friedmann's 1922 solutions showed expanding or contracting universes without it. Edwin Hubble's 1929 redshift observations confirmed expansion, leading Einstein to drop the static model and call Λ his "greatest blunder," per George Gamow.[50] This led to the Friedmann–Lemaître–Robertson–Walker metric for an expanding universe from a hot, dense start. Today, Λ returns as dark energy speeding expansion, though its cause remains unknown.[51]

Quantum Physics Engagements

Contributions to Old Quantum Theory

Einstein contributed to early quantum theory by applying quantization to light, matter, and radiation. In 1905, he explained the photoelectric effect—where light ejects electrons from a metal surface only if its frequency exceeds a threshold, regardless of intensity—by proposing that light consists of discrete energy packets called light quanta.[52] This idea extended Max Planck's 1900 quantization of energy exchanges to the electromagnetic field, suggesting light has particle-like properties that challenge classical wave theory.[53] Robert Millikan's experiments from 1914 to 1916 verified Einstein's formula for electron kinetic energy as proportional to frequency minus the work function (minimum energy to free an electron). This work earned Einstein the 1921 Nobel Prize in Physics for the photoelectric law.[52] In 1907, Einstein extended quantum ideas to matter with a model for the specific heat of solids—the energy needed to raise their temperature. He treated atoms as independent quantum harmonic oscillators with discrete energy levels En=(n+1/2)hνE_n = (n + 1/2) h \nu, where hh is Planck's constant and ν\nu is a characteristic frequency.[54] At low temperatures, this model predicted specific heat CVC_V approaches zero, as oscillators enter ground states and stop absorbing heat. It fixed the classical Dulong-Petit law's failure to account for low-temperature drops.[55] Peter Debye later refined it with a continuum model for phonon dispersion, but Einstein's approach pioneered quantization in solid thermal properties.[53] In 1917, Einstein advanced radiation theory by linking absorption, spontaneous emission, and stimulated emission—where incoming light triggers an excited atom to emit identical photons. He introduced coefficients AA (spontaneous) and BB (stimulated and absorption) for transition probabilities in atoms interacting with blackbody radiation.[56] Stimulated processes depend linearly on radiation energy density, predicting lasers and masers decades later.[57] This framework connected quantum discreteness to thermodynamic balance and influenced ideas like Bohr's correspondence principle, though Einstein saw it as provisional without deeper mechanics.[53]

Objections to Quantum Mechanics and Determinism

Einstein rejected the probabilistic interpretation of quantum mechanics, maintaining that the theory's apparent indeterminism reflected its incompleteness rather than a fundamental feature of reality. He argued that physical reality should possess definite attributes independent of measurement, and that quantum mechanics failed to provide a complete description because it predicted outcomes only in terms of probabilities rather than precise predictions.[58] This stance stemmed from his commitment to classical determinism, where the state of the universe at any time fully determines its future evolution via local causal laws, without inherent randomness.[59]
Albert Einstein and Niels Bohr walking together
Albert Einstein (left) and Niels Bohr, whose debates at the 1927 and 1930 Solvay Conferences centered on quantum mechanics and determinism
In a 1926 letter to Max Born, Einstein expressed this view metaphorically, stating, "I, at any rate, am convinced that He [God] does not throw dice," critiquing Born's probabilistic formulation of quantum transitions as abandoning objective reality for statistical ensembles.[60] He elaborated during the 1927 Solvay Conference that quantum mechanics' reliance on observer-dependent probabilities undermined the goal of physics to describe an objective, independent reality, proposing thought experiments like the "clock in a box" to challenge the uncertainty principle's universality.[61] Niels Bohr countered these by refining the complementarity principle, asserting that wave-particle duality inherently limits simultaneous knowledge of conjugate variables, but Einstein persisted, viewing such resolutions as evasive of deeper causal structures.[61] The debates continued at the 1930 Solvay Conference, where Einstein's photon box gedankenexperiment aimed to evade Heisenberg's uncertainty relation, only for Bohr to rebut it using general relativity's time dilation effects.[61] Einstein's most formal objection appeared in the 1935 EPR paper, co-authored with Boris Podolsky and Nathan Rosen, titled "Can Quantum-Mechanical Description of Physical Reality Be Considered Complete?" They considered entangled particles, such as two electrons in a spin-singlet state separated by large distances, where measuring one instantly determines the other's properties with certainty, implying either non-local influences violating relativity's locality or pre-existing "elements of reality" that quantum mechanics failed to predict.[62] Einstein labeled this "spooky action at a distance" as untenable, arguing quantum mechanics must be incomplete, supplanted by a deterministic theory incorporating hidden variables to restore local realism.[62] Despite Bohr's response emphasizing the formalism's consistency without hidden causes, Einstein upheld that true theories must yield definite, local predictions for all observables, influencing later pursuits like Bohmian mechanics, though he never endorsed non-local alternatives.[63]

EPR Paradox and Philosophical Debates with Niels Bohr

In 1935, Albert Einstein, Boris Podolsky, and Nathan Rosen published a paper questioning the completeness of quantum mechanics (QM). Titled "Can Quantum-Mechanical Description of Physical Reality Be Considered Complete?", it appeared in Physical Review and introduced the EPR paradox.[64] The paradox describes entangled particles—linked so that measuring one's position or momentum instantly fixes the other's, even across vast distances.[63] Einstein and his co-authors argued that QM's failure to predict these properties beforehand implies either no objective reality independent of measurement (rejecting realism) or faster-than-light influences (violating locality). Both options seemed unacceptable. They concluded QM needs hidden variables—unseen factors—to fully describe reality, as it cannot assign definite values to all observables without disturbing the system.[62][65]
Albert Einstein and Niels Bohr in conversation
Einstein and Bohr during one of their discussions on quantum mechanics
Niels Bohr responded in June 1935. He defended the Copenhagen interpretation, which views QM as complete. Bohr argued that EPR wrongly applied classical ideas to quantum events. In QM, measurement alters the system, and properties like position and momentum cannot both have fixed values at once. He saw no need for hidden variables, treating QM's probabilities as basic limits on what we can know, linked to the idea of complementarity and the role of measuring tools.[63] These ideas deepened a long-standing philosophical divide. It began at the 1927 Solvay Conference, where Einstein used thought experiments to probe QM's limits, and continued at the 1930 conference, where Bohr highlighted how measurements define quantum context.[68] Einstein favored local realism and determinism. He rejected QM's chance-based outcomes—famously saying "God does not play dice"—and sought a theory that kept special relativity's locality and objective traits before any measurement, avoiding "spooky action at a distance."[58][66] Bohr, in contrast, pointed to QM's strong predictions and dropped classical realism for quantum scales. He preferred complementary views over hidden unified causes.[67][68] The debates lasted until Einstein's death in 1955. They contrasted his push for determinism with Bohr's acceptance of indeterminism. Einstein's challenges, including advanced thought experiments, found no flaws in QM. Yet the EPR paradox inspired later work, like Bell's theorem in the 1960s, which tested locality through experiments.[67]

Advanced Theoretical Efforts

Unified Field Theory Pursuits

Einstein began pursuing a unified field theory in the mid-1920s to combine the gravitational field of general relativity with electromagnetism in a single classical geometric framework. This effort drew on spacetime curvature's success in gravity, hoping electromagnetism would emerge from a broader metric. His first explicit reference to the term appeared in a 1925 paper, "Unified Field Theory," presented to the Prussian Academy of Sciences on October 15. It used an asymmetric affine connection to link gravity and electromagnetism while maintaining general covariance, but mathematical issues like non-integrable connections led to quick abandonment.[68][69]
Handwritten manuscript page by Albert Einstein with German text and equations
Manuscript page signed by Albert Einstein featuring mathematical notes and diagrams
From 1925 until his death in 1955, Einstein published at least eleven papers on the topic, often working alone at the Institute for Advanced Study in Princeton. Key attempts included the 1928–1929 teleparallelism theory, which used torsion instead of curvature to describe gravity and aimed to incorporate electromagnetism, but failed to match observations without adjustments. In the 1930s and 1940s, he explored five-dimensional extensions inspired by Kaluza-Klein, as in a 1938 paper, yet faced challenges with dimensional reduction and stability. His final effort, the 1950 non-symmetric theory developed from 1945 to 1953, employed asymmetric metric and connection tensors to model fields and particles as field singularities, viewing matter as deterministic self-interactions rather than quantum probabilities.[69][70][71][72]
Open book with title page dedicated to Albert Einstein
Title page of 'Geometry of Einstein's Unified Field Theory' by Václav Hlavatý, dedicated to the memory of Albert Einstein
These theories produced no testable predictions matching experiments, such as new particles or forces. Their classical, non-quantum nature clashed with quantum electrodynamics' successes and ignored phenomena like electron spin or nuclear forces. Despite critiques from physicists like Wolfgang Pauli on the quantum disconnect, Einstein continued, favoring a deterministic local field theory over probabilistic interpretations.[73][68][74]

Other Investigations and Collaborations

Einstein collaborated with his Institute for Advanced Study assistant Nathan Rosen on the Einstein-Rosen bridge, a 1935 general relativity model linking two exterior Schwarzschild regions via a narrow throat to eliminate the black hole singularity. Motivated by an atomistic view of matter and electricity without discontinuities, it detailed in their Physical Review paper an early effort to geometrize elementary particles as extended field configurations rather than points.[75][76] From 1936 to 1938, the pair studied gravitational waves, initially submitting a paper arguing that such disturbances do not propagate to infinity due to coordinate singularities. They withdrew it after Rosen identified the error; the corrected version confirmed wave propagation, resolving skepticism from exact solutions.[77] Einstein worked with Leopold Infeld and Banesh Hoffmann to solve general relativity's "problem of motion," deriving the 1938 Einstein-Infeld-Hoffmann equations. These approximate trajectories of multiple compact bodies from vacuum field equations alone, avoiding Newtonian assumptions while yielding post-Newtonian orbital terms.[76] With assistant Peter Bergmann from 1936, Einstein explored fifth-dimensional formalisms in 1938, promoting a coordinate-free, four-dimensional approach to unified theories through higher-dimensional metric projections. These efforts produced no complete synthesis.[78] The collaborations reflected Einstein's emphasis on field-derived dynamics over quantum probabilistic methods, favoring causal determinism in gravity.[79]

Emigration, War, and Later Career

Escape from Nazi Europe

In December 1932, amid the rising influence of the Nazi Party in Germany, Albert Einstein left Berlin for a planned lecture tour at the California Institute of Technology in the United States.[80] When Adolf Hitler became Chancellor on January 30, 1933, Einstein—already in the US—condemned the regime's antisemitic policies and refused to return.[81] Nazi authorities soon raided his Berlin properties and Caputh summer house, seizing papers and vandalizing the site.[80]
Einstein's Swiss passport, issued in June 1923
Einstein's Swiss passport open to the identification page with his photograph and personal details
Einstein moved to Belgium in early 1933 to stay with family, resigning from the Prussian Academy of Sciences on March 28 due to its submission to Nazi pressure.[82] On March 10, he renounced German citizenship for the second time—first in 1896 to evade military service—writing to a friend, "I will not be returning to Germany, perhaps never again," as Nazi agents plotted his assassination with a bounty.[83] [84] To escape threats, he hid in a remote Norfolk cottage in England for three weeks in April 1933.[85]
Albert Einstein on the deck of a ship
Einstein arriving in the United States aboard ship in October 1933
Einstein arrived permanently in the United States on October 17, 1933, aboard the Belgenland, settling in Princeton, New Jersey, at the newly founded Institute for Advanced Study.[86] His Swiss citizenship and academic connections eased the move, despite Nazi propaganda branding him a fugitive and decrying his work as "Jewish physics."[80] This departure severed his ties to Nazi-controlled Europe; he never returned.[87]

Settlement in the United States

Following his departure from Europe amid rising Nazi persecution, Albert Einstein arrived in the United States on October 17, 1933, aboard the Belgenland from Antwerp, Belgium, entering as a refugee.[88][89] He had renounced his German citizenship earlier that year, becoming stateless, and proceeded directly to Princeton, New Jersey, with his wife Elsa.[3][82] Einstein accepted a lifetime research position at the newly founded Institute for Advanced Study (IAS) in Princeton, joining as one of its inaugural Faculty members in the School of Mathematics, where he remained until his death in 1955.[90] The IAS, established in 1930 by donors Louis Bamberger and Caroline Bamberger Fuld, offered an environment for uninterrupted theoretical work without teaching obligations, suiting Einstein's focus on inquiry over administration.[91] Upon arrival, he and Elsa stayed temporarily at the Peacock Inn while securing permanent housing.[92]
Two-story white frame house with porch and shutters
Albert Einstein's home at 112 Mercer Street in Princeton, New Jersey
In August 1935, Einstein purchased a two-story frame house at 112 Mercer Street, which became his primary residence until death, initially shared with Elsa Einstein, secretary Helen Dukas, and occasional family.[93][94] The modest home near the IAS reflected his unpretentious lifestyle despite fame, though admirers prompted a privacy fence.[92]
Albert Einstein and two women raising hands during citizenship oath
Einstein taking the oath of U.S. citizenship in Trenton, New Jersey, October 1940, with stepdaughter Margot and secretary Helen Dukas
Einstein obtained U.S. naturalized citizenship on October 1, 1940, in Trenton, New Jersey, alongside stepdaughter Margot Einstein and Helen Dukas, while retaining his 1901 Swiss citizenship.[5][99] This dual status highlighted ties to Switzerland, but his work in Princeton centered on unified field theories and public discourse.[100]

World War II, Manhattan Project, and Postwar Stances

Einstein renounced absolute pacifism after the Nazi rise and supported the Allied effort through anti-fascism advocacy and fundraising, including manuscript auctions.[80] His opposition stemmed from Nazi persecution of Jews and scientists, prompting warnings about weaponizing scientific advances.[95]
Albert Einstein and Leo Szilard examining a document
Einstein with Leo Szilard, who drafted the 1939 letter to President Roosevelt warning of nuclear fission risks
In August 1939, Einstein signed a letter drafted by Leo Szilard, with input from Edward Teller and Eugene Wigner, addressed to President Franklin D. Roosevelt on October 11. It highlighted nuclear fission research and Germany's potential to build powerful uranium bombs.[96][97] Prompted by German nuclear intelligence, the letter urged U.S. research acceleration and uranium reserves, contributing to the Advisory Committee on Uranium and the Manhattan Project.[98]
Women operating control panels at Y-12 plant in Oak Ridge
Calutron operators at the Y-12 electromagnetic separation plant, part of the Manhattan Project's Oak Ridge facility
Einstein's indirect role ended there; the U.S. Army denied him security clearance in July 1940 due to his pacifist past, leftist associations, and German origins, citing espionage risks.[99][100] He lacked involvement in project operations or advance knowledge of the August 1945 Hiroshima and Nagasaki bombings.[101] Postwar, Einstein called the 1939 letter his "one great mistake," regretting it after learning Germany failed to build a bomb and anticipating a nuclear arms race beyond defense.[102] Still, he saw the bombs as speeding Japan's surrender and avoiding a bloodier invasion, while cautioning their existential danger—estimating in 1945 that future nuclear war could kill two-thirds of humanity without destroying civilization entirely.[103] He pushed for nuclear disarmament and international control, co-founding the 1946 Emergency Committee of Atomic Scientists to raise awareness of atomic risks and promote civilian energy oversight.[104] In 1955, Einstein backed the Russell-Einstein Manifesto, which warned of nuclear threats to humanity and urged peaceful conflict resolution, helping spawn the Pugwash Conferences.[105] He opposed U.S. hydrogen bomb development in 1949–1950, advising President Truman it would heighten tensions, and advocated supranational authority over atomic weapons.[104]

Personal Life and Character

Marriages, Relationships, and Family Dynamics

Mileva Marić and Albert Einstein, 1912
Albert Einstein with his first wife Mileva Marić in 1912
Einstein married twice. His first wife was Mileva Marić, a physics student he met at the Swiss Federal Polytechnic in Zurich in the late 1890s. They wed on January 6, 1903, in Bern, Switzerland.[106][107] Before marrying, Marić gave birth to their daughter Lieserl Einstein on January 27, 1902, in Novi Sad, Serbia. Lieserl died of scarlet fever in September 1903, at about 21 months old.[108][109] The couple had two sons: Hans Albert Einstein, born May 14, 1904, in Bern, and Eduard Einstein, born July 28, 1910, in Zurich.[110][111] Einstein's career demands and emotional distance strained the marriage. In July 1914, Marić moved to Zurich with the sons while Einstein remained in Berlin.[112] That year, he suggested they live together under harsh rules—no intimacy, obedience to him, and minimal contact—which she refused, prompting separation.[113] They divorced on February 14, 1919, after five years apart. The agreement gave Marić any Nobel Prize money, which she received in 1921: about 125,000 Swiss francs for Einstein's photoelectric effect award.[114] Einstein began an affair around 1912 with his cousin Elsa Löwenthal, a divorced mother of two daughters, Ilse (born 1897) and Margot (born 1899).[115] They married on June 2, 1919, in Berlin. Elsa managed the home, shielded him from interruptions, and traveled with him, providing stability until her death from heart and kidney failure on December 20, 1936.[116] He viewed Ilse and Margot as stepdaughters and grew close to Margot, even proposing marriage to her in 1918 (she declined).[117] Letters released in 2006 reveal Einstein's extramarital affairs during both marriages, including with secretary Betty Neumann and at least five other women. He called their affection "unwanted" despite his flirtations.[118][119] After divorcing Marić, he sent financial aid for her and the sons' living and education costs, but emotional relations stayed tense.[110] Hans Albert pursued engineering against Einstein's wish for pure science, sparking conflicts. Einstein opposed his 1927 marriage to Frieda Knecht, 18 years younger, and briefly cut support. Hans Albert moved to the United States in 1938, became a hydraulic engineering professor at the University of California, Berkeley, and had four children.[120] Eduard showed early talent in literature and psychiatry but developed schizophrenia around age 20, diagnosed in 1930. He lived in Zurich's Burghölzli clinic from 1932 until dying of a stroke on October 25, 1965.[111][121] Einstein expressed concern in letters but visited rarely, focusing on work as the condition worsened.[111] Marić cared for Eduard until her 1948 death; state care followed.[122]

Daily Habits, Interests, and Personality Traits

Albert Einstein seated at a desk writing with a pen
Albert Einstein engaged in thoughtful work at his desk
Einstein followed a structured daily routine balancing intellectual work, rest, and physical activity. He slept about ten hours nightly, took short daytime naps for mental clarity, and started mornings with breakfast around 9–10 a.m., newspaper reading, and focused work until early afternoon.[123][124] Afternoons featured continued home study after lunch and a brief tea break.[125] He often walked the 1.5-mile distance to the Institute for Advanced Study in Princeton, using strolls for contemplation rather than rushed travel. He observed that "The monotony and solitude of a quiet life stimulates the creative mind," a personal reflection shared in his 1933 speech "Civilization and Science" at the Royal Albert Hall in London.[126] Music was central among his interests; Einstein played the violin regularly to unwind and process scientific ideas.[127] Sailing provided another pursuit, enjoyed despite his inability to swim and incidents of capsizing or disorientation, offering escape from daily pressures.[128] He avoided socks due to foot swelling and adopted vegetarianism later for animal welfare reasons.[129]
Albert Einstein outdoors with tousled white hair and mustache
Albert Einstein in later years outdoors
Einstein's personality blended intellectual curiosity with rebellion against authority, often showing impudence toward rigid conventions.[130] Biographers highlight his expansive imagination and humility—attributing success to curiosity rather than innate superiority—tempered by occasional arrogance in debates.[131] Absent-minded in daily matters, such as losing his way while sailing, he displayed generosity, humanitarian concern, and personal simplicity.[130] His wit, self-deprecating humor, and strong independence resisted dogmatic institutions.[132]

Intellectual and Ideological Views

Political Positions and Critiques of Collectivism

Einstein supported socialist principles. He criticized capitalism for creating economic oligarchy, exploiting workers, and causing crises through private ownership of production. In his May 1949 essay "Why Socialism?" in Monthly Review, he argued that unchecked capital accumulation leads to elite monopolies that prioritize profit over societal needs, resulting in inequality.[133] He advocated a planned economy with collective ownership of production means. This system would be democratically coordinated to secure livelihoods. He stressed education to counter individualism and decentralized bodies to protect liberty.[134] His democratic socialism rejected market liberalism's "anarchic" competition, which he blamed for social problems like dehumanizing labor and speculative finance. Einstein backed economic collectivism through workers' cooperatives and state intervention against monopolies. In the 1930s, during the Great Depression, he called for public control of key industries.[135] He opposed laissez-faire economics, saying its profit motive turned human relations into commodities and deepened class divisions. These issues appeared in interwar wage gaps and industrial conflicts in Europe and the United States.[136] Still, he warned that socialist planning required democratic safeguards to avoid bureaucratic tyranny, drawing from risks in centralized systems.[137] Einstein rejected authoritarian collectivism. He condemned Nazism as nationalism combined with totalitarian control, which sacrificed individual autonomy to racial ideals of the volk. In a 1930 interview, he dismissed National Socialism as temporary. But by 1932, he urged resistance to fascism's rise, especially after Adolf Hitler's January 1933 appointment as chancellor, which crushed dissent and science.[81] The regime burned his books and offered a bounty on his life, prompting his emigration and attacks on fascism as anti-reason and anti-humanist.[138] Einstein initially viewed the 1917 Bolshevik Revolution as an egalitarian experiment fitting social evolution, despite its coercive methods.[139] By the 1930s, Joseph Stalin's purges and trials, which killed millions, led him to criticize suppressed freedoms. He argued true socialism needed open debate, not one-party rule.[140] In 1953, during McCarthyism, he defended communists' rights against loyalty oaths but rejected Marxist dogmatism. He preferred voluntary cooperation over enforced uniformity to prevent totalitarianism, whether fascist or Stalinist, and placed human welfare above ideology.[141][142]

Religious Skepticism and Philosophical Realism

Scan of letter from Guy Raner to Albert Einstein
Guy H. Raner, Jr.'s letter to Einstein, June 1945, questioning his religious views
Einstein doubted organized religion and a personal God. He saw these beliefs as responses to human needs, not facts. In a 1954 letter to philosopher Eric Gutkind, he described "God" as "nothing more than the expression and product of human weaknesses" and the Bible as a "collection of honorable, but still primitive legends which are nevertheless pretty childish."[143] He dismissed ideas of a God who rewards or punishes as childish superstition.[144] Einstein avoided strict atheism. Instead, he followed a cosmic religious sense from Baruch Spinoza. Here, "God" meant the universe's orderly harmony, not a being who acts on human lives. In a 1929 interview, he said: "I believe in Spinoza's God who reveals himself in the orderly harmony of what exists, not in a God who concerns himself with fates and actions of human beings."[145] This view fit with science, which uncovers real patterns. Faith-based ideas, he argued, block clear understanding.[146] Raised in a secular Jewish home with rational influences, Einstein skipped religious practices. He criticized religious groups for pushing dogma over evidence.[147]
Scan of Albert Einstein's reply letter to Guy Raner
Einstein's letter to Guy Raner, September 1949, rejecting a personal God as childlike
Einstein's outlook matched his scientific realism. He believed physical reality exists on its own, ruled by fixed cause-and-effect laws, not chance. This drove his doubts about quantum mechanics' core ideas. In the 1935 Einstein-Podolsky-Rosen paper with Boris Podolsky and Nathan Rosen, he claimed quantum rules implied either instant links across distances—which break relativity—or that the theory misses real properties like position and momentum until measured.[148] Einstein rejected instrumentalism, like Niels Bohr's approach, which treats theories as mere tools. He demanded theories describe a real, cause-driven world that tests can reach. His famous line, "God does not play dice with the universe," rejected the Copenhagen interpretation's role for chance. He sought hidden factors to bring back clear causes and local effects.[148] Quantum tests matched predictions, but Einstein insisted true knowledge needs realism. This shaped debates in physics' foundations and upheld a cosmos of rational order.[149] The quote "Reality is merely an illusion, albeit a very persistent one" is often linked to Einstein but is a loose summary. It comes from his March 21, 1955, letter to Michele Besso's family: "For us believing physicists, the distinction between past, present, and future is only a stubbornly persistent illusion." This ties to relativity's block universe, where all times exist together. The common version extends this time idea to all reality.[150]

Views on Zionism, Nationalism, and Internationalism

Letter from Albert Einstein dated January 21, 1946
Einstein's 1946 letter discussing Palestine as a bi-national homeland rather than a separate Jewish state
Einstein supported cultural Zionism, focused on Jewish spiritual and communal revival, initially with reservations but by the 1920s viewing it as a means of ending Jewish discrimination and "pariah status."[151][152] He helped found the Hebrew University of Jerusalem, which opened in 1925, raising funds, delivering its first scientific lecture, and leaving his papers and literary rights to its archives.[154][155] He argued a Jewish homeland in Palestine would allow Jews to shape public life by their own ideals and provide Diaspora Jews with moral support and communal identity.[153][156] He backed a Jewish refuge in Palestine for persecuted Jews, testifying before the Anglo-American Committee of Inquiry in 1946 and defending the Balfour Declaration in a 1947 letter to Nehru as a historically just allocation of ancestral land.[152][158] Upon Israel's declaration of independence in 1948 he described it as "the fulfillment of our dreams."[159] He credited Zionism with reviving Jewish communal cohesion and providing survivors of persecution the dignity to endure it.[160] Yet Einstein opposed an exclusive Jewish state with borders, army, or power over Arabs. He favored a binational commonwealth with equal Jewish-Arab rights under one parliament.[151] In 1948, he rejected fundraising for the Stern Gang due to their terrorism, like the Deir Yassin massacre.[152] In 1930, he opposed partitioning Palestine into Jewish and Arab states, saying it would harm Jewish settlement's moral base by favoring separation over coexistence.[153] In 1952, after Chaim Weizmann's death, he declined Israel's presidency, stating he was deeply moved by the offer from our State of Israel but cited his lack of political experience and poor skills in dealing with people.[154] At his 1955 death, he was writing a speech for Israel's seventh anniversary to air on TV.[155] His 1948 letter targeted Zionist extremism, while his 1952 reply focused on his leadership limits. Einstein criticized nationalism as "an infantile disease" like "the measles of mankind," linking it to tragedies such as World War II.[156] He rejected all forms, including hidden patriotism, as sources of unfair privileges by group that bred injustice and war.[157] Nazi German nationalism shaped this view, which he saw as a spreading illness causing militarism and fear of outsiders. He separated it from protective cultural ties, like Jewish survival.[158] In 1936 letters to Louis Brandeis, he said Jewish endurance came from ethics and intellect, not a nationalist state in Palestine.[158] Einstein pushed internationalism via a world government to enforce peace and limit states' war powers. After World War II, he shifted from full pacifism—held before 1933—to federalism, where nations gave way to global rule. He argued lasting sovereignty fueled arms races and rivalries, dooming peace.[159] In 1946, he backed a world government holding force monopoly, focused on stopping wars while allowing cultural and economic freedom. Without it, he warned, atomic bombs threatened human survival.[156] He saw this as the fix for nationalism's harms, noting groups like the United Nations lacked real power.[160]

Controversies and Disputes

Priority Claims and Plagiarism Accusations

Portraits of Albert Einstein (left) and David Hilbert (right)
Albert Einstein and David Hilbert, the key figures in the 1915 general relativity priority dispute
Critics have accused Albert Einstein of plagiarism in his development of special relativity. These claims focus on his 1905 paper. There, detractors say he used ideas from Hendrik Lorentz and Henri Poincaré without enough credit. Lorentz created the Lorentz transformations in 1904. He aimed to explain the null result of the Michelson–Morley experiment. Poincaré, from 1900 to 1905, explored relativity of simultaneity and length contraction. He coined those terms. Einstein derived the transformations on his own. He started from two postulates of relativity. Yet he left out direct mentions of his predecessors. This led Philipp Lenard to call it plagiarism in the 1920s. Lenard won the Nobel Prize in 1905. Later, he supported Nazi views and labeled relativity "Jewish science." His attacks fit into broader antisemitic pushback.[161] Historians of science counter these claims. They note Einstein's key innovation. He combined prior ideas into a framework without the ether. This extended the principle of relativity to all laws of physics. It went beyond fixes for electromagnetism. Poincaré kept absolute time and an undetectable ether. Einstein used an axiomatic approach. It led to new results, like reciprocal time dilation. Tests of E=mc² support his original unification. Citation gaps matched norms in theoretical physics then. They do not show deliberate theft. Fringe claims of direct copying come from unverified sources. These lack backing from original documents.[162][163]
Historical documents of gravitational field equations by Einstein and Hilbert, November 1915
First pages of the 1915 papers on general relativity field equations: Einstein's submission dated November 25 (left) and Hilbert's related work (right)
A priority dispute arose in 1915 between Einstein and David Hilbert. Hilbert submitted a paper on November 20. It included field equations like Einstein's final version. Einstein presented his on November 25 to the Prussian Academy of Sciences. Einstein visited Göttingen in October. There, mathematician Hilbert worked with him. Hilbert wanted help to ground his theory in physics. Hilbert's paper stressed unifying gravitation and electromagnetism. It used variational principles. He credited Einstein's physical insights. Later versions named Einstein as the theory's source. Archives show Einstein derived his work independently. It built on the equivalence principle from 1907. Hilbert assumed general covariance too soon. Experts agree Einstein provided the core concepts. Hilbert sped up the math. This solved Mercury's perihelion shift through physical steps, not just math.[164][165][166] Claims of plagiarism in the photoelectric effect are rare and lack proof. Einstein won the 1921 Nobel Prize for it. His 1905 explanation introduced light quanta. These eject electrons based on frequency. He extended Max Planck's idea beyond blackbody radiation. Robert Millikan's 1916 experiments confirmed it. Broader charges, from Lenard or modern critics, often confuse shared progress with stealing. They ignore Einstein's thought experiments and original notes. These disputes highlight tensions between building on prior work and full originality. Yet mainstream history views Einstein as the architect of relativity.[167][168]

Inconsistencies in Pacifism and Scientific Advocacy

![Einstein's letter to President Roosevelt urging atomic research, dated August 2, 1939][float-right] Einstein upheld pacifism in his early career, opposing militarism and nationalism before World War I and signing anti-war manifestos during it.[169] The rise of Nazism, however, led him to abandon absolute pacifism; after fleeing Germany in 1933, he endorsed armed resistance against the regime, diverging from pacifist peers who opposed all violence.[80] This change stemmed from viewing Hitler's expansionism as an overriding threat requiring defensive measures.[170] In 1939, Einstein signed a letter drafted by Leo Szilard to President Franklin D. Roosevelt, alerting him to Nazi potential for nuclear weapons via uranium fission and urging U.S. research into chain reactions for military use.[171] [98] Dated August 2, it spurred the Advisory Committee on Uranium, precursor to the Manhattan Project. This support for weaponizing science clashed with his prior aversion to military applications, motivated by concern over German dominance.[171] After the war, Einstein regretted the letter, telling Linus Pauling in 1954 it was "the one great mistake in my life," given Germany's limited progress and the U.S. bombs' civilian toll in Japan.[102] [172] He then opposed nuclear proliferation, co-authoring the 1955 Russell-Einstein Manifesto calling for weapons abolition and global cooperation, while backing world federalism to limit national arms control.[105] [104] These actions reflected a qualified return to pacifism, acknowledging science's dual potential, amid tensions between ideals and wartime realities. His endorsement of defensive science, without direct bomb involvement, highlighted conflicts between pure research advocacy and its strategic use against existential dangers like Nazism.[173]

Xenophobic Entries in Travel Diaries

Book cover of The Travel Diaries of Albert Einstein
The Travel Diaries of Albert Einstein: The Far East, Palestine & Spain, 1922–1923, edited by Ze'ev Rosenkranz
Einstein's private travel diaries from his 1922–1923 lecture tour of Asia, including China and Japan, contain xenophobic and racist remarks, particularly derogatory stereotypes about Chinese people, such as describing them as "industrious, filthy, obtuse little people" and a "herd-like nation" lacking individuality. These entries, intended for personal use and not public dissemination at the time, were published in the 2018 edition edited by Ze'ev Rosenkranz, revealing prejudices that contrast with Einstein's later public opposition to racism and ethnocentrism.[174]

Surveillance and Political Persecutions

After the Nazis seized power in January 1933, Einstein—a Jewish physicist who opposed nationalism and militarism—faced persecution in Germany. Stormtroopers raided his Caputh summer home shortly after Adolf Hitler's appointment as chancellor, and officials offered a 15,000 Reichsmark reward for information on his assassination. Einstein had renounced his German citizenship that year while in the United States. He denounced the regime as a "return to barbarism," refused to return, and entered exile. Nazi media, such as Kladderadatsch, depicted him as a racial inferior and agitator in antisemitic attacks on Jewish intellectuals.[175][87] En route to the United States, Einstein hid briefly in a Norfolk coastal hut in England in August 1933, arranged by Commander Oliver Locker-Lampson amid assassination threats. Public reports of plots prompted a move for safety. He reached the United States on October 17, 1933, aboard the Conte Grande, welcomed as a refugee from fascism, though his pacifist and socialist views drew official attention.[85] From December 1932 until his death in 1955, the Federal Bureau of Investigation (FBI) under J. Edgar Hoover surveilled Einstein, gathering over 1,400 declassified pages. Agents monitored his calls, mail, trash, and contacts, suspecting communist links due to his backing of pacifist groups, world government ideas, and outfits like the National Committee for a Sane Foreign Policy—a group labeled a communist front. Informants alleged Soviet connections, but records revealed no subversive actions; the watch arose from Cold War and McCarthy-era suspicions, with Hoover failing to deport him because of Einstein's stature.[176][177] At the height of McCarthyism in the early 1950s, Einstein criticized House Un-American Activities Committee (HUAC) inquiries as a grave threat to freedom. He urged W. E. B. Du Bois and Bertrand Russell to reject testimony on principle instead of citing the Fifth Amendment. Never subpoenaed himself, his views drew charges of disloyalty from anti-communists, including Senator Joseph McCarthy, who deemed him an enemy of America. Continued FBI scrutiny of his Zionism and anti-nuclear positions exposed conflicts between his civil liberties defense and state security measures, with files mostly holding unproven claims.[178][179][180]

Death and Enduring Legacy

Final Years, Illness, and Death

Einstein's desk with papers, books, and blackboard equations
Albert Einstein's desk at the Institute for Advanced Study, photographed the day after his death in 1955
In his final years, Albert Einstein lived in Princeton, New Jersey, and continued research at the Institute for Advanced Study after retiring in 1945. He pursued a unified field theory to unify general relativity and electromagnetism, without success, while advocating against nuclear proliferation.[90][181] Einstein knew of his cardiovascular problems since 1948, when surgeons at Princeton Hospital treated an expanding abdominal aortic aneurysm by wrapping the aorta with cellophane to prevent rupture, extending his life despite complications. He ignored advice to stop smoking, often using his pipe and salvaging tobacco scraps—a known aneurysm risk factor.[182][183] On April 17, 1955, severe abdominal pain from the aneurysm's rupture struck Einstein at home, causing internal hemorrhage. At Princeton Hospital, he refused surgery from leading physicians, stating, "I want to go when I want. It is tasteless to prolong life artificially. I have done my share; it is time to go. I will do it elegantly." He received morphine and continued light work, such as dictating notes.[182][184]
Hands holding preserved sections of Einstein's brain
Preserved sections of Albert Einstein's brain after removal and study
Einstein died early on April 18, 1955, at age 76, after speaking German words to his nurse whose meaning was lost in translation. The autopsy confirmed death by ruptured aneurysm. Pathologist Thomas Harvey removed and preserved the brain without family consent for study, sectioning it into 240 blocks, creating hundreds of slides, photographing it, and sharing pieces with researchers; some later went missing. The body was cremated, with ashes scattered at an undisclosed site as Einstein wished.[184][182][185][186]

Scientific Confirmations and Modern Challenges

Einstein's general theory of relativity, published in 1915, has faced repeated tests that confirm its predictions. It forecasted that the Sun's gravity would bend starlight. Expeditions led by Arthur Eddington and Andrew Crommelin observed this during the May 29, 1919, solar eclipse, measuring a deflection of about 1.75 arcseconds—matching general relativity but exceeding Newtonian expectations.[187] The theory also explained Mercury's perihelion anomaly, the unexplained advance of the planet's closest orbital point to the Sun. It predicted an extra 43 arcseconds per century beyond Newtonian calculations, a shift later verified by observations.[188] Another forecast, gravitational redshift—the shift of light to longer wavelengths as it escapes a gravitational field—was tested in the 1959 Pound–Rebka experiment. Using gamma rays, it detected frequency changes matching general relativity, with later tests achieving higher precision.[188] Modern experiments provide further support. Gravitational waves, ripples in spacetime from massive accelerating objects, were first detected by LIGO on September 14, 2015, from a black hole merger 1.3 billion light-years away. The waveforms matched general relativity simulations within 1% for amplitude and phase. Later events, including GW250114 in January 2025—the strongest signal to date—tested the theory in intense gravity fields, confirming predictions like black hole ringdown and Hawking's area theorem.[47][189] Special relativity's time dilation, where time slows for fast-moving objects, appears in cosmic ray muons that live longer than expected and in GPS satellites, which need corrections for speed and gravity to prevent daily errors of about 10 km.[190] Frame-dragging, the twisting of spacetime by a rotating body like Earth, was measured by Gravity Probe B. Launched in 2004, it used orbiting gyroscopes to detect geodetic precession to 0.28% accuracy and frame-dragging to 19% accuracy.[191] Challenges remain where general relativity meets quantum mechanics, such as at black hole centers or the Big Bang's origin, where the theory predicts infinities but quantum effects dominate. Einstein's attempts at a classical unified field theory from the 1920s to 1955 aimed to merge gravity and electromagnetism deterministically. These efforts ignored quantum advances and lacked testable results, partly due to his rejection of quantum probabilities.[74] The cosmological constant, introduced in 1917 for a static universe and later dubbed Einstein's "greatest blunder" after Hubble's 1929 discovery of expansion, now explains the universe's accelerating growth as dark energy, which makes up about 68% of total energy density. Yet its tiny observed value conflicts with quantum estimates by 120 orders of magnitude, creating the cosmological constant problem.[192] Recent data, like 2024 weak lensing surveys hinting at small deviations from general relativity on large scales (under 5-sigma confidence) and the Hubble constant mismatch—local measurements at ~73 km/s/Mpc versus cosmic microwave background values of ~67 km/s/Mpc—suggest possible refinements or errors, but do not refute the theory.[193][194] General relativity excels in weak fields like the solar system but requires quantum gravity extensions for extreme conditions.

Broader Cultural and Societal Influence

Albert Einstein in old age
Albert Einstein in his later years, with his iconic wild hair and expressive face
Einstein's image as an absent-minded genius, marked by wild hair and an expressive face, shaped popular culture. It led to portrayals of him as an eccentric scientist in films, television, and ads.[195] [196] This trope began in his lifetime and continued after his death. Examples include Walter Matthau as a matchmaking Einstein in the 1994 film I.Q. and animated versions in Rick and Morty and Young Einstein.[197] [198] His equation E=mc²—energy equals mass times the speed of light squared—stands as a symbol of scientific genius. Media often uses it to suggest deep insight, even if few grasp the full theory of relativity.[199] [200] Einstein boosted public interest in science. He remains history's most famous scientist, linking theoretical physics to progress.[200] [201] His 1931 visit to the United States, where he met stars like Charlie Chaplin, mixed science with celebrity. This shaped views of intellectuals in democracies.[197] Einstein's writings influenced education. He criticized rote learning and pushed for independent thinking and imagination. In 1952, he wrote that too much focus on facts kills curiosity, calling schools trainers of "a mass of slaves who think they are free."[202] His ideas supported reforms favoring creativity over memorization.[201] As a Jewish refugee from Nazi Germany, he highlighted immigrants' role in innovation. This challenged ideas of cultural sameness and showed how exiles aid host countries.[203] [204] His humanism promoted rational ethics in society, though views differed by ideology.[205][206] Among the many quotes misattributed to Einstein is "Creativity is contagious, pass it on," which has no basis in his documented statements. The phrase first appeared in the 1977 book Creative Growth Games and was erroneously linked to Einstein starting in a 1992 advertisement. Quote Investigator

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