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Theoretical physics
Theoretical physics
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Visual representation of a Schwarzschild wormhole. Wormholes have never been observed, but they are predicted to exist through mathematical models and scientific theory.

Theoretical physics is a branch of physics that employs mathematical models and abstractions of physical objects and systems to rationalize, explain, and predict natural phenomena. This is in contrast to experimental physics, which uses experimental tools to probe these phenomena.

The advancement of science generally depends on the interplay between experimental studies and theory. In some cases, theoretical physics adheres to standards of mathematical rigour while giving little weight to experiments and observations.[a] For example, while developing special relativity, Albert Einstein was concerned with the Lorentz transformation which left Maxwell's equations invariant, but was apparently uninterested in the Michelson–Morley experiment on Earth's drift through a luminiferous aether.[1] Conversely, Einstein was awarded the Nobel Prize for explaining the photoelectric effect, previously an experimental result lacking a theoretical formulation.[2]

Overview

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A physical theory is a model of physical events. It is judged by the extent to which its predictions agree with empirical observations. The quality of a physical theory is also judged on its ability to make new predictions which can be verified by new observations. A physical theory differs from a mathematical theorem in that while both are based on some form of axioms, judgment of mathematical applicability is not based on agreement with any experimental results.[3][4] A physical theory similarly differs from a mathematical theory, in the sense that the word "theory" has a different meaning in mathematical terms.[b]

The equations for an Einstein manifold, used in general relativity to describe the curvature of spacetime

A physical theory involves one or more relationships between various measurable quantities. Archimedes realized that a ship floats by displacing its mass of water, Pythagoras understood the relation between the length of a vibrating string and the musical tone it produces.[5][6] Other examples include entropy as a measure of the uncertainty regarding the positions and motions of unseen particles and the quantum mechanical idea that (action and) energy are not continuously variable.[citation needed]

Theoretical physics consists of several different approaches. In this regard, theoretical particle physics forms a good example. For instance: "phenomenologists" might employ (semi-) empirical formulas and heuristics to agree with experimental results, often without deep physical understanding.[c] "Modelers" (also called "model-builders") often appear much like phenomenologists, but try to model speculative theories that have certain desirable features (rather than on experimental data), or apply the techniques of mathematical modeling to physics problems.[d] Some attempt to create approximate theories, called effective theories, because fully developed theories may be regarded as unsolvable or too complicated. Other theorists may try to unify, formalise, reinterpret or generalise extant theories, or create completely new ones altogether.[e] Sometimes the vision provided by pure mathematical systems can provide clues to how a physical system might be modeled;[f] e.g., the notion, due to Riemann and others, that space itself might be curved. Theoretical problems that need computational investigation are often the concern of computational physics.

Theoretical advances may consist in setting aside old, incorrect paradigms (e.g., aether theory of light propagation, caloric theory of heat, burning consisting of evolving phlogiston, or astronomical bodies revolving around the Earth) or may be an alternative model that provides answers that are more accurate or that can be more widely applied. In the latter case, a correspondence principle will be required to recover the previously known result.[7][8] Sometimes though, advances may proceed along different paths. For example, an essentially correct theory may need some conceptual or factual revisions; atomic theory, first postulated millennia ago (by several thinkers in Greece and India) and the two-fluid theory of electricity[9] are two cases in this point. However, an exception to all the above is the wave–particle duality, a theory combining aspects of different, opposing models via the Bohr complementarity principle.

Relationship between mathematics and physics

Physical theories become accepted if they are able to make correct predictions and no (or few) incorrect ones. The theory should have, at least as a secondary objective, a certain economy and elegance (compare to mathematical beauty), a notion sometimes called "Occam's razor" after the 13th-century English philosopher William of Occam (or Ockham), in which the simpler of two theories that describe the same matter just as adequately is preferred (but conceptual simplicity may mean mathematical complexity).[10] They are also more likely to be accepted if they connect a wide range of phenomena. Testing the consequences of a theory is part of the scientific method.[11]

Physical theories can be grouped into three categories: mainstream theories, proposed theories and fringe theories.[citation needed]

History

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Theoretical physics began at least 2,300 years ago, under the pre-Socratic philosophy, and continued by Plato and Aristotle, whose views held sway for a millennium. During the rise of medieval universities, the only acknowledged intellectual disciplines were the seven liberal arts of the Trivium like grammar, logic, and rhetoric and of the Quadrivium like arithmetic, geometry, music and astronomy. During the Middle Ages and Renaissance, the concept of experimental science, the counterpoint to theory, began with scholars such as Ibn al-Haytham and Francis Bacon. As the Scientific Revolution gathered pace, the concepts of matter, energy, space, time and causality slowly began to acquire the form we know today, and other sciences spun off from the rubric of natural philosophy. Thus began the modern era of theory with the Copernican paradigm shift in astronomy, soon followed by Johannes Kepler's expressions for planetary orbits, which summarized the meticulous observations of Tycho Brahe; the works of these men (alongside Galileo's) can perhaps be considered to constitute the Scientific Revolution.[citation needed]

The great push toward the modern concept of explanation started with Galileo Galilei, one of the few physicists who was both a consummate theoretician and a great experimentalist. The analytic geometry and mechanics of René Descartes were incorporated into the calculus and mechanics of Isaac Newton, another theoretician/experimentalist of the highest order, writing Principia Mathematica.[12] In it contained a grand synthesis of the work of Copernicus, Galileo and Kepler; as well as Newton's theories of mechanics and gravitation, which held sway as worldviews until the early 20th century. Simultaneously, progress was also made in optics (in particular colour theory and the ancient science of geometrical optics), courtesy of Newton, Descartes and the Dutchmen Willebrord Snell and Christiaan Huygens. In the 18th and 19th centuries Joseph-Louis Lagrange, Leonhard Euler and William Rowan Hamilton would extend the theory of classical mechanics considerably.[13] They picked up the interactive intertwining of mathematics and physics begun two millennia earlier by Pythagoras.[citation needed]

Among the great conceptual achievements of the 19th and 20th centuries were the consolidation of the idea of energy (as well as its global conservation) by the inclusion of heat, electricity and magnetism, and then light. Lord Kelvin and Walther Nernst's discoveries of the laws of thermodynamics, and more importantly Rudolf Clausius's introduction of the singular concept of entropy, began to provide a macroscopic explanation for the properties of matter. Statistical mechanics (followed by statistical physics and quantum statistical mechanics) emerged as an offshoot of thermodynamics late in the 19th century. Another important event in the 19th century was James Clerk Maxwell's discovery of electromagnetic theory, unifying the previously separate phenomena of electricity, magnetism and light.[citation needed]

The pillars of modern physics, and perhaps the most revolutionary theories in the history of physics, have been relativity theory, devised by Albert Einstein, and quantum mechanics, founded by Werner Heisenberg, Max Born, Pascual Jordan, and Erwin Schrödinger. Newtonian mechanics was subsumed under special relativity and Newton's gravity was given a kinematic explanation by general relativity. Quantum mechanics led to an understanding of blackbody radiation (which indeed, was an original motivation for the theory) and of anomalies in the specific heats of solids — and finally to an understanding of the internal structures of atoms and molecules. Quantum mechanics soon gave way to the formulation of quantum field theory (QFT), begun in the late 1920s. In the aftermath of World War II, more progress brought much renewed interest in QFT, which had since the early efforts, stagnated. The same period also saw fresh attacks on the problems of superconductivity and phase transitions, as well as the first applications of QFT in the area of theoretical condensed matter. The 1960s and 70s saw the formulation of the Standard Model of particle physics using QFT and progress in condensed matter physics (theoretical foundations of superconductivity and critical phenomena, among others), in parallel to the applications of relativity to problems in astronomy and cosmology respectively.[citation needed]

All of these achievements depended on the theoretical physics as a moving force both to suggest experiments and to consolidate results — often by ingenious application of existing mathematics, or, as in the case of Descartes and Newton (with Leibniz), by inventing new mathematics. Fourier's studies of heat conduction led to a new branch of mathematics: infinite, orthogonal series.[14]

Modern theoretical physics attempts to unify theories and explain phenomena in further attempts to understand the Universe, from the cosmological to the elementary particle scale. Where experimentation cannot be done, theoretical physics still tries to advance through the use of mathematical models.[citation needed]

Mainstream theories

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Mainstream theories (sometimes referred to as central theories) are the body of knowledge of both factual and scientific views and possess a usual scientific quality of the tests of repeatability, consistency with existing well-established science and experimentation. There do exist mainstream theories that are generally accepted theories based solely upon their effects explaining a wide variety of data, although the detection, explanation, and possible composition are subjects of debate.[citation needed]

Examples

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Proposed theories

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The proposed theories of physics are usually relatively new theories which deal with the study of physics which include scientific approaches, means for determining the validity of models and new types of reasoning used to arrive at the theory. However, some proposed theories include theories that have been around for decades and have eluded methods of discovery and testing. Proposed theories can include fringe theories in the process of becoming established (and, sometimes, gaining wider acceptance). Proposed theories usually have not been tested. In addition to the theories like those listed below, there are also different interpretations of quantum mechanics, which may or may not be considered different theories since it is debatable whether they yield different predictions for physical experiments, even in principle. For example, AdS/CFT correspondence, Chern–Simons theory, graviton, magnetic monopole, string theory, theory of everything.[citation needed]

Fringe theories

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Fringe theories include any new area of scientific endeavor in the process of becoming established and some proposed theories. It can include speculative sciences. This includes physics fields and physical theories presented in accordance with known evidence, and a body of associated predictions have been made according to that theory.[citation needed]

Some fringe theories go on to become a widely accepted part of physics. Other fringe theories end up being disproven. Some fringe theories are a form of protoscience and others are a form of pseudoscience. The falsification of the original theory sometimes leads to reformulation of the theory.[citation needed]

Examples

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Thought experiments vs real experiments

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"Thought" experiments are situations created in one's mind, asking a question akin to "suppose you are in this situation, assuming such is true, what would follow?". They are usually created to investigate phenomena that are not readily experienced in every-day situations. Famous examples of such thought experiments are Schrödinger's cat, the EPR thought experiment, simple illustrations of time dilation, and so on. These usually lead to real experiments designed to verify that the conclusion (and therefore the assumptions) of the thought experiments are correct. The EPR thought experiment led to the Bell inequalities, which were then tested to various degrees of rigor, leading to the acceptance of the current formulation of quantum mechanics and probabilism as a working hypothesis.[citation needed]

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
Theoretical physics is the subfield of physics dedicated to interpreting and codifying experimental data into a coherent body of , known as , to explain and predict the behavior of physical systems in the . It relies on abstract models, computations, and conceptual frameworks rather than direct experimentation to rationalize natural phenomena, drawing on disciplines such as , , astronomy, , chemistry, and geology. Theoretical physicists develop hypotheses and predictive models that guide , often exploring fundamental questions about the origins and structure of , , , and time. The historical roots of theoretical physics trace back to in the , but the modern field crystallized in the early amid crises in , leading to revolutionary developments in quantum theory and relativity. Quantum theory began in 1900 when proposed that energy is emitted in discrete quanta to resolve the problem, a Einstein extended in 1905 to explain the using light quanta (photons), for which he received the 1921 . Concurrently, Einstein's special , published in 1905, unified space and time into and established the equivalence of mass and energy (E=mc²), addressing inconsistencies between Newtonian mechanics and . This culminated in the 1915 formulation of , which redefined as the curvature of caused by mass and energy, profoundly influencing cosmology and . Contemporary theoretical physics encompasses diverse branches, including , which provides the mathematical framework for the of elementary particles and their interactions; for gravitational phenomena; and condensed matter theory for understanding solids, liquids, and complex materials. Efforts to unify these frameworks persist, notably in , which posits that fundamental particles are vibrating strings in higher dimensions, and quantum gravity approaches aiming to reconcile with relativity. Theoretical physicists employ advanced methods such as vector analysis, differential equations, Fourier transforms, , and numerical simulations to model systems ranging from subatomic particles to the cosmos. These theories not only predict observable effects, like confirmed in 2015, but also drive technological innovations and deepen our comprehension of the universe's fundamental laws.

Definition and Scope

Core Definition

Theoretical physics is the branch of physics that employs mathematical abstractions, hypotheses, and logical reasoning to explain and predict physical phenomena, focusing on constructing abstract models of natural laws rather than direct empirical testing. This approach emphasizes the development of conceptual frameworks that capture the underlying principles governing the universe, allowing physicists to derive consequences from assumed axioms and compare them with observable outcomes. Key characteristics of theoretical physics include its reliance on deductive methods, where conclusions are logically inferred from foundational premises, and the use of idealized models to simplify complex systems for analysis. Examples of such models include point particles, which treat objects as having zero spatial extent to facilitate calculations in mechanics and particle physics, and continuous fields, which represent forces like electromagnetism as smooth distributions across space rather than discrete entities. Additionally, theoretical physics prioritizes the universality of laws, seeking principles that apply consistently across all scales and conditions, independent of specific local contexts. The term "theoretical physics" emerged in the 19th century, particularly in German-speaking academic circles, to delineate this deductive, model-based pursuit from the more applied or experimentally oriented aspects of the discipline. Its scope encompasses phenomena from the subatomic realm, such as the strong interactions described by , to vast cosmic structures governed by , unifying diverse scales under a coherent theoretical umbrella.

Distinction from Experimental Physics

Theoretical physics primarily involves the development of mathematical models and hypotheses to explain and predict physical phenomena, relying on from abstract principles rather than direct observation. In contrast, focuses on designing and conducting measurements to collect empirical data, testing hypotheses through controlled observations and instrumentation. The two fields are interdependent, with theoretical models guiding experimental design by specifying what phenomena to investigate or predict outcomes to verify. For instance, the was theoretically predicted in 1964 as part of the electroweak symmetry-breaking mechanism in the , directing experimental searches at particle accelerators. Conversely, experimental results can refine or falsify theories; the 1887 Michelson-Morley experiment's null result, which failed to detect the luminiferous ether, undermined classical ether theories and paved the way for . Philosophically, theoretical physics employs the hypothetico-deductive method, where hypotheses are formulated and logical consequences are derived to make testable predictions. , however, often utilizes , generalizing broader principles from accumulated specific observations and data patterns. A key challenge in distinguishing the fields arises from computational simulations, which blend theoretical modeling with experimental-like validation by numerically solving equations to mimic real-world systems, often serving as a bridge between pure prediction and empirical testing.

Historical Development

Ancient and Classical Foundations

The foundations of theoretical physics trace back to ancient philosophical inquiries into the nature of motion and change, particularly among Greek thinkers. Aristotle (384–322 BCE), in his work Physics, proposed a teleological framework where natural phenomena are explained through four causes: material (the substance composing an object), formal (its structure or essence), efficient (the agent producing change), and final (its purpose or end goal). He distinguished natural motion—such as the downward fall of earth or upward rise of fire—as inherent to elements seeking their "natural place," contrasting it with violent motion imposed by external forces. This qualitative approach dominated early conceptions of dynamics, influencing subsequent thought for over a millennium. Building on Aristotelian ideas, (c. 287–212 BCE) advanced quantitative methods in through his treatises and On the Equilibrium of Planes. In , he formulated the principle that a body immersed in a fluid experiences an upward buoyant force equal to the weight of the displaced fluid, enabling precise calculations for floating objects and laying groundwork for . His work on levers established the as inversely proportional to the distances from the fulcrum, expressed as the equilibrium condition where moments balance: for weights w1w_1 and w2w_2 at distances d1d_1 and d2d_2, w1d1=w2d2w_1 d_1 = w_2 d_2. These contributions shifted focus toward mathematical rigor in analyzing forces and equilibrium. During the medieval period, Islamic scholars refined observational and analytical techniques, bridging ancient and modern paradigms. (c. 965–1040 CE), in his , pioneered an experimental methodology by systematically testing hypotheses on propagation, , and reflection, demonstrating that travels in straight lines from objects to the eye and refuting emission theories of vision. His controlled experiments with pinhole cameras and lenses emphasized repeatable observations, prefiguring the in and laying empirical foundations for later physical theories. In , (c. 1320–1382) introduced graphical representations of motion in his Tractatus de configurationibus qualitatum et motuum, plotting against time to visualize uniform as a linear increase, allowing qualitative proofs of mean speed theorems without algebraic notation. This innovation facilitated conceptual analysis of changing qualities like speed, influencing kinematic thought. The marked a pivotal shift toward empirical and mathematical modeling of motion. (1564–1642), in (1638), developed by studying inclined planes and pendulums, establishing that objects in accelerate uniformly regardless of mass and introducing the concept of : bodies maintain uniform motion in the absence of friction or external forces. His resolution of trajectories into horizontal (constant ) and vertical (accelerated) components provided a vectorial framework for dynamics. Complementing this, (1571–1630) derived his three laws of planetary motion from Tycho Brahe's precise astronomical data (1546–1601), published in (1609) and Harmonices Mundi (1619): planets orbit the Sun in ellipses with the Sun at one focus; a line from the Sun to a planet sweeps equal areas in equal times (indicating conserved angular momentum); and the square of the orbital period is proportional to the cube of the semi-major axis (T2a3T^2 \propto a^3). These empirical laws challenged geocentric models and demanded a unified theoretical explanation. Isaac Newton's (1687) synthesized these developments into a comprehensive mechanical framework. Newton unified terrestrial and celestial motion through his three laws of motion—first stating , second relating to (F=maF = ma), and third describing action-reaction pairs—and his law of universal gravitation, positing that every mass attracts every other with a proportional to the product of their masses and inversely proportional to the square of their separation: F=Gm1m2r2F = G \frac{m_1 m_2}{r^2} where GG is the gravitational constant. By demonstrating that Kepler's laws follow from this inverse-square force applied to elliptical orbits, Newton established a deterministic, mathematical basis for classical mechanics, transforming theoretical physics into a predictive science.

19th and Early 20th Century Advances

The 19th century marked a pivotal shift in theoretical physics toward unifying disparate phenomena through mathematical frameworks, building upon classical mechanics to address heat, electricity, and magnetism. In thermodynamics, Sadi Carnot introduced the concept of an ideal heat engine in 1824, describing a reversible cycle that maximizes work output from heat transfer between reservoirs at different temperatures, laying the groundwork for the second law of thermodynamics. This model, analyzed without knowledge of energy conservation, emphasized efficiency limits based on temperature differences. Rudolf Clausius formalized entropy in 1865 as a state function quantifying irreversible processes, defined mathematically as S=dQrevTS = \int \frac{dQ_{\text{rev}}}{T}, where dQrevdQ_{\text{rev}} is reversible heat transfer and TT is absolute temperature, establishing that entropy increases in isolated systems. Ludwig Boltzmann advanced this in the late 19th century through statistical mechanics, linking macroscopic thermodynamic properties to microscopic particle states; his 1877 formula S=klnWS = k \ln W, with kk as Boltzmann's constant and WW as the number of microstates, probabilistically explained entropy as a measure of disorder, bridging atomic chaos to observable irreversibility. Electromagnetism saw profound unification with James Clerk Maxwell's 1865 equations, a set of four partial differential equations that integrated electric and magnetic fields into a single electromagnetic field theory, predicting that changing electric fields generate magnetic fields and vice versa. These equations implied the existence of electromagnetic waves propagating at speed c=1ϵ0μ0c = \frac{1}{\sqrt{\epsilon_0 \mu_0}}
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