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Hydrogen in its plasma state is the most abundant ordinary matter in the universe.

In classical physics and general chemistry, matter is any substance that has mass and takes up space by having volume.[1] All everyday objects that can be touched are ultimately composed of atoms, which are made up of interacting subatomic particles. In everyday as well as scientific usage, matter generally includes atoms and anything made up of them, and any particles (or combination of particles) that act as if they have both rest mass and volume. However it does not include massless particles such as photons, or other energy phenomena or waves such as light or heat.[1]: 21 [2] Matter exists in various states (also known as phases). These include classical everyday phases such as solid, liquid, and gas – for example water exists as ice, liquid water, and gaseous steam – but other states are possible, including plasma, Bose–Einstein condensates, fermionic condensates, and quark–gluon plasma.[3]

Usually atoms can be imagined as a nucleus of protons and neutrons, and a surrounding "cloud" of orbiting electrons which "take up space".[4][5] However, this is only somewhat correct because subatomic particles and their properties are governed by their quantum nature, which means they do not act as everyday objects appear to act – they can act like waves as well as particles, and they do not have well-defined sizes or positions. In the Standard Model of particle physics, matter is not a fundamental concept because the elementary constituents of atoms are quantum entities which do not have an inherent "size" or "volume" in any everyday sense of the word. Due to the exclusion principle and other fundamental interactions, some "point particles" known as fermions (quarks, leptons), and many composites and atoms, are effectively forced to keep a distance from other particles under everyday conditions; this creates the property of matter which appears to us as matter taking up space.

For much of the history of the natural sciences, people have contemplated the exact nature of matter. The idea that matter was built of discrete building blocks, the so-called particulate theory of matter, appeared in both ancient Greece and ancient India.[6] Early philosophers who proposed the particulate theory of matter include the Indian philosopher Kaṇāda (c. 6th century BCE),[7] and the pre-Socratic Greek philosophers Leucippus (c. 490 BCE) and Democritus (c. 470–380 BCE).[8]

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Comparison with mass

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Matter is a general term describing any physical substance, which is sometimes defined in incompatible ways in different fields of science. Some definitions are based on historical usage from a time when there was no reason to distinguish mass from simply a quantity of matter. By contrast, mass is not a substance but a well-defined, extensive property of matter and other substances or systems. Various types of mass are defined within physics – including rest mass, inertial mass, and relativistic mass.

In physics, matter is sometimes equated with particles that exhibit rest mass (i.e., that cannot travel at the speed of light), such as quarks and leptons. However, in both physics and chemistry, matter exhibits both wave-like and particle-like properties (the so-called wave–particle duality).[9][10][11]

Relation with chemical substance

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Tuff
Steam and liquid water are two different forms of the same pure chemical substance, water.
Tuff
Picture of a formed molecule

A chemical substance is a unique form of matter with constant chemical composition and characteristic properties.[12][13] Chemical substances may take the form of a single element or chemical compounds. If two or more chemical substances can be combined without reacting, they may form a chemical mixture.[14] If a mixture is separated to isolate one chemical substance to a desired degree, the resulting substance is said to be chemically pure.[15]

Chemical substances can exist in several different physical states or phases (e.g. solids, liquids, gases, or plasma) without changing their chemical composition. Substances transition between these phases of matter in response to changes in temperature or pressure. Some chemical substances can be combined or converted into new substances by means of chemical reactions. Chemicals that do not possess this ability are said to be inert.

Pure water is an example of a chemical substance, with a constant composition of two hydrogen atoms bonded to a single oxygen atom (i.e. H2O). The atomic ratio of hydrogen to oxygen is always 2:1 in every molecule of water. Pure water will tend to boil near 100 °C (212 °F), an example of one of the characteristic properties that define it. Other notable chemical substances include diamond (a form of the element carbon), table salt (NaCl; an ionic compound), and refined sugar (C12H22O11; an organic compound).

Definition

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Based on atoms

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A definition of "matter" based on its physical and chemical structure is: matter is made up of atoms.[16] Such atomic matter is also sometimes termed ordinary matter. As an example, deoxyribonucleic acid molecules (DNA) are matter under this definition because they are made of atoms. This definition can be extended to include charged atoms and molecules, so as to include plasmas (gases of ions) and electrolytes (ionic solutions), which are not obviously included in the atoms definition. Alternatively, one can adopt the protons, neutrons, and electrons definition.

Based on protons, neutrons and electrons

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A definition of "matter" more fine-scale than the atoms and molecules definition is: matter is made up of what atoms and molecules are made of, meaning anything made of positively charged protons, neutral neutrons, and negatively charged electrons.[17] This definition goes beyond atoms and molecules, however, to include substances made from these building blocks that are not simply atoms or molecules, for example, electron beams in an old cathode ray tube television, or white dwarf matter—typically, carbon and oxygen nuclei in a sea of degenerate electrons. At a microscopic level, the constituent "particles" of matter such as protons, neutrons, and electrons obey the laws of quantum mechanics and exhibit wave-particle duality. At an even deeper level, protons and neutrons are made up of quarks and the force fields (gluons) that bind them together, leading to the next definition.

Based on quarks and leptons

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Under the "quarks and leptons" definition, the elementary and composite particles made of the quarks (in purple) and leptons (in green) would be matter—while the gauge bosons (in red) would not be matter. However, interaction energy inherent to composite particles (for example, gluons involved in neutrons and protons) contribute to the mass of ordinary matter.

As seen in the above discussion, many early definitions of what can be called "ordinary matter" were based on its structure or "building blocks". On the scale of elementary particles, a definition that follows this tradition can be stated as: "ordinary matter is everything that is composed of quarks and leptons", or "ordinary matter is everything that is composed of any elementary fermions except antiquarks and antileptons".[18][19][20] The connection between these formulations follows.

Leptons (the most famous being the electron), and quarks (of which baryons, such as protons and neutrons, are made) combine to form atoms, which in turn form molecules. Because atoms and molecules are said to be matter, it is natural to phrase the definition as: "ordinary matter is anything that is made of the same things that atoms and molecules are made of". (However, notice that one also can make from these building blocks matter that is not atoms or molecules.) Then, because electrons are leptons, and protons and neutrons are made of quarks, this definition in turn leads to the definition of matter as being "quarks and leptons", which are two of the four types of elementary fermions (the other two being antiquarks and antileptons, which can be considered antimatter as described later). Carithers and Grannis state: "Ordinary matter is composed entirely of first-generation particles, namely the [up] and [down] quarks, plus the electron and its neutrino."[19] (Higher generations particles quickly decay into first-generation particles, and thus are not commonly encountered.[21])

This definition of ordinary matter is more subtle than it first appears. All the particles that make up ordinary matter (leptons and quarks) are elementary fermions, while all the force carriers are elementary bosons.[22] The W and Z bosons that mediate the weak force are not made of quarks or leptons, and so are not ordinary matter, even if they have mass.[23] In other words, mass is not something that is exclusive to ordinary matter.

The quark–lepton definition of ordinary matter, however, identifies not only the elementary building blocks of matter, but also includes composites made from the constituents (atoms and molecules, for example). Such composites contain an interaction energy that holds the constituents together, and may constitute the bulk of the mass of the composite. As an example, to a great extent, the mass of an atom is simply the sum of the masses of its constituent protons, neutrons and electrons. However, digging deeper, the protons and neutrons are made up of quarks bound together by gluon fields (see dynamics of quantum chromodynamics) and these gluon fields contribute significantly to the mass of hadrons.[24] In other words, most of what composes the "mass" of ordinary matter is due to the binding energy of quarks within protons and neutrons.[25] For example, the sum of the mass of the three quarks in a nucleon is approximately 12.5 MeV/c2, which is low compared to the mass of a nucleon (approximately 938 MeV/c2).[26][27] The bottom line is that most of the mass of everyday objects comes from the interaction energy of its elementary components.

The Standard Model groups matter particles into three generations, where each generation consists of two quarks and two leptons. The first generation is the up and down quarks, the electron and the electron neutrino; the second includes the charm and strange quarks, the muon and the muon neutrino; the third generation consists of the top and bottom quarks and the tau and tau neutrino.[28] The most natural explanation for this would be that quarks and leptons of higher generations are excited states of the first generations. If this turns out to be the case, it would imply that quarks and leptons are composite particles, rather than elementary particles.[29]

This quark–lepton definition of matter also leads to what can be described as "conservation of (net) matter" laws—discussed later below. Alternatively, one could return to the mass–volume–space concept of matter, leading to the next definition, in which antimatter becomes included as a subclass of matter.

Based on elementary fermions (mass, volume, and space)

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A common or traditional definition of matter is "anything that has mass and volume (occupies space)".[30][31] For example, a car would be said to be made of matter, as it has mass and volume (occupies space).

The observation that matter occupies space goes back to antiquity. However, an explanation for why matter occupies space is recent, and is argued to be a result of the phenomenon described in the Pauli exclusion principle,[32][33] which applies to fermions. Two particular examples where the exclusion principle clearly relates matter to the occupation of space are white dwarf stars and neutron stars, discussed further below.

Thus, matter can be defined as everything composed of elementary fermions. Although we do not encounter them in everyday life, antiquarks (such as the antiproton) and antileptons (such as the positron) are the antiparticles of the quark and the lepton, are elementary fermions as well, and have essentially the same properties as quarks and leptons, including the applicability of the Pauli exclusion principle which can be said to prevent two particles from being in the same place at the same time (in the same state), i.e. makes each particle "take up space". This particular definition leads to matter being defined to include anything made of these antimatter particles as well as the ordinary quark and lepton, and thus also anything made of mesons, which are unstable particles made up of a quark and an antiquark.

In general relativity and cosmology

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In the context of relativity, mass is not an additive quantity, in the sense that one cannot add the rest masses of particles in a system to get the total rest mass of the system.[1]: 21  In relativity, usually a more general view is that it is not the sum of rest masses, but the energy–momentum tensor that quantifies the amount of matter. This tensor gives the rest mass for the entire system. Matter, therefore, is sometimes considered as anything that contributes to the energy–momentum of a system, that is, anything that is not purely gravity.[34][35] This view is commonly held in fields that deal with general relativity such as cosmology. In this view, light and other massless particles and fields are all part of matter.

Structure

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In particle physics, fermions are particles that obey Fermi–Dirac statistics. Fermions can be elementary, like the electron—or composite, like the proton and neutron. In the Standard Model, there are two types of elementary fermions: quarks and leptons, which are discussed next.

Quarks

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Quarks are massive particles of spin-12, implying that they are fermions. They carry an electric charge of −13 e (down-type quarks) or +23 e (up-type quarks). For comparison, an electron has a charge of −1 e. They also carry colour charge, which is the equivalent of the electric charge for the strong interaction. Quarks also undergo radioactive decay, meaning that they are subject to the weak interaction.

Quark properties[36]
name symbol spin electric charge
(e)
mass
(MeV/c2)
mass comparable to antiparticle antiparticle
symbol
up-type quarks
up u 12 +23 1.5 to 3.3 ~ 5 electrons antiup u
charm c 12 +23 1160 to 1340 ~ 1 proton anticharm c
top t 12 +23 169,100 to 173,300 ~ 180 protons or
~1 tungsten atom
antitop t
down-type quarks
down d 12 13 3.5 to 6.0 ~10 electrons antidown d
strange s 12 13 70 to 130 ~ 200 electrons antistrange s
bottom b 12 13 4130 to 4370 ~ 5 protons antibottom b

Baryonic

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Quark structure of a proton: 2 up quarks and 1 down quark.

Baryons are strongly interacting fermions, and so are subject to Fermi–Dirac statistics. Amongst the baryons are the protons and neutrons, which occur in atomic nuclei, but many other unstable baryons exist as well. The term baryon usually refers to triquarks—particles made of three quarks. Also, "exotic" baryons made of four quarks and one antiquark are known as pentaquarks, but their existence is not generally accepted.

Baryonic matter is the part of the universe that is made of baryons (including all atoms). This part of the universe does not include dark energy, dark matter, black holes or various forms of degenerate matter, such as those that compose white dwarf stars and neutron stars. Microwave light seen by Wilkinson Microwave Anisotropy Probe (WMAP) suggests that only about 4.6% of that part of the universe within range of the best telescopes (that is, matter that may be visible because light could reach us from it) is made of baryonic matter. About 26.8% is dark matter, and about 68.3% is dark energy.[37]

The great majority of ordinary matter in the universe is unseen, since visible stars and gas inside galaxies and clusters account for less than 10 per cent of the ordinary matter contribution to the mass–energy density of the universe.[38]

Hadronic

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Hadronic matter can refer to 'ordinary' baryonic matter, made from hadrons (baryons and mesons), or quark matter (a generalisation of atomic nuclei), i.e. the 'low' temperature QCD matter.[39] It includes degenerate matter and the result of high energy heavy nuclei collisions.[40]

Degenerate

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In physics, degenerate matter refers to the ground state of a gas of fermions at a temperature near absolute zero.[41] The Pauli exclusion principle requires that only two fermions can occupy a quantum state, one spin-up and the other spin-down. Hence, at zero temperature, the fermions fill up sufficient levels to accommodate all the available fermions—and in the case of many fermions, the maximum kinetic energy (called the Fermi energy) and the pressure of the gas becomes very large, and depends on the number of fermions rather than the temperature, unlike normal states of matter.

Degenerate matter is thought to occur during the evolution of heavy stars.[42] The demonstration by Subrahmanyan Chandrasekhar that white dwarf stars have a maximum allowed mass because of the exclusion principle caused a revolution in the theory of star evolution.[43]

Degenerate matter includes the part of the universe that is made up of neutron stars and white dwarfs.

Strange

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Strange matter is a particular form of quark matter, usually thought of as a liquid of up, down, and strange quarks. It is contrasted with nuclear matter, which is a liquid of neutrons and protons (which themselves are built out of up and down quarks), and with non-strange quark matter, which is a quark liquid that contains only up and down quarks. At high enough density, strange matter is expected to be color superconducting. Strange matter is hypothesized to occur in the core of neutron stars, or, more speculatively, as isolated droplets that may vary in size from femtometers (strangelets) to kilometers (quark stars).

Two meanings
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In particle physics and astrophysics, the term is used in two ways, one broader and the other more specific.

  1. The broader meaning is just quark matter that contains three flavors of quarks: up, down, and strange. In this definition, there is a critical pressure and an associated critical density, and when nuclear matter (made of protons and neutrons) is compressed beyond this density, the protons and neutrons dissociate into quarks, yielding quark matter (probably strange matter).
  2. The narrower meaning is quark matter that is more stable than nuclear matter. The idea that this could happen is the "strange matter hypothesis" of Bodmer[44] and Witten.[45] In this definition, the critical pressure is zero: the true ground state of matter is always quark matter. The nuclei that we see in the matter around us, which are droplets of nuclear matter, are actually metastable, and given enough time (or the right external stimulus) would decay into droplets of strange matter, i.e. strangelets.

Leptons

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Leptons are particles of spin-12, meaning that they are fermions. They carry an electric charge of −1 e (charged leptons) or 0 e (neutrinos). Unlike quarks, leptons do not carry colour charge, meaning that they do not experience the strong interaction. Leptons also undergo radioactive decay, meaning that they are subject to the weak interaction. Leptons are massive particles, therefore are subject to gravity.

Lepton properties
name symbol spin electric charge
(e)
mass
(MeV/c2)
mass comparable to antiparticle antiparticle
symbol
charged leptons[46]
electron e
12 −1 0.5110 1 electron antielectron e+
muon μ
12 −1 105.7 ~ 200 electrons antimuon μ+
tau τ
12 −1 1,777 ~ 2 protons antitau τ+
neutrinos[47]
electron neutrino ν
e
12 0 < 0.000460 < 11000 electron electron antineutrino ν
e
muon neutrino ν
μ
12 0 < 0.19 < 12 electron muon antineutrino ν
μ
tau neutrino ν
τ
12 0 < 18.2 < 40 electrons tau antineutrino ν
τ

Phases

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Phase diagram for a typical substance at a fixed volume

In bulk, matter can exist in several different forms, or states of aggregation, known as phases,[48] depending on ambient pressure, temperature and volume.[49] A phase is a form of matter that has a relatively uniform chemical composition and physical properties (such as density, specific heat, refractive index, and so forth). These phases include the three familiar ones (solids, liquids, and gases), as well as more exotic states of matter (such as plasmas, superfluids, supersolids, Bose–Einstein condensates, ...). A fluid may be a liquid, gas or plasma. There are also paramagnetic and ferromagnetic phases of magnetic materials. As conditions change, matter may change from one phase into another. These phenomena are called phase transitions and are studied in the field of thermodynamics. In nanomaterials, the vastly increased ratio of surface area to volume results in matter that can exhibit properties entirely different from those of bulk material, and not well described by any bulk phase (see nanomaterials for more details).

Phases are sometimes called states of matter, but this term can lead to confusion with thermodynamic states. For example, two gases maintained at different pressures are in different thermodynamic states (different pressures), but in the same phase (both are gases).

Antimatter

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Unsolved problem in physics
Baryon asymmetry. Why is there far more matter than antimatter in the observable universe?

Antimatter is matter that is composed of the antiparticles of those that constitute ordinary matter. If a particle and its antiparticle come into contact with each other, the two annihilate; that is, they may both be converted into other particles with equal energy in accordance with Albert Einstein's equation E = mc2. These new particles may be high-energy photons (gamma rays) or other particle–antiparticle pairs. The resulting particles are endowed with an amount of kinetic energy equal to the difference between the rest mass of the products of the annihilation and the rest mass of the original particle–antiparticle pair, which is often quite large. Depending on which definition of "matter" is adopted, antimatter can be said to be a particular subclass of matter, or the opposite of matter.

Antimatter is not found naturally on Earth, except very briefly and in vanishingly small quantities (as the result of radioactive decay, lightning or cosmic rays). This is because antimatter that came to exist on Earth outside the confines of a suitable physics laboratory would almost instantly meet the ordinary matter that Earth is made of, and be annihilated. Antiparticles and some stable antimatter (such as antihydrogen) can be made in tiny amounts, but not in enough quantity to do more than test a few of its theoretical properties.

There is considerable speculation both in science and science fiction as to why the observable universe is apparently almost entirely matter (in the sense of quarks and leptons but not antiquarks or antileptons), and whether other places are almost entirely antimatter (antiquarks and antileptons) instead. In the early universe, it is thought that matter and antimatter were equally represented, and the disappearance of antimatter requires an asymmetry in physical laws called CP (charge–parity) symmetry violation, which can be obtained from the Standard Model,[50] but at this time the apparent asymmetry of matter and antimatter in the visible universe is one of the great unsolved problems in physics. Possible processes by which it came about are explored in more detail under baryogenesis.

Formally, antimatter particles can be defined by their negative baryon number or lepton number, while "normal" (non-antimatter) matter particles have positive baryon or lepton number.[51] These two classes of particles are the antiparticle partners of one another.

In October 2017, scientists reported further evidence that matter and antimatter, equally produced at the Big Bang, are identical, should completely annihilate each other and, as a result, the universe should not exist.[52] This implies that there must be something, as yet unknown to scientists, that either stopped the complete mutual destruction of matter and antimatter in the early forming universe, or that gave rise to an imbalance between the two forms.

Conservation

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Two quantities that can define an amount of matter in the quark–lepton sense (and antimatter in an antiquark–antilepton sense), baryon number and lepton number, are conserved in the Standard Model. A baryon such as the proton or neutron has a baryon number of one, and a quark, because there are three in a baryon, is given a baryon number of 1/3. So the net amount of matter, as measured by the number of quarks (minus the number of antiquarks, which each have a baryon number of −1/3), which is proportional to baryon number, and number of leptons (minus antileptons), which is called the lepton number, is practically impossible to change in any process. Even in a nuclear bomb, none of the baryons (protons and neutrons of which the atomic nuclei are composed) are destroyed—there are as many baryons after as before the reaction, so none of these matter particles are actually destroyed and none are even converted to non-matter particles (like photons of light or radiation). Instead, nuclear (and perhaps chromodynamic) binding energy is released, as these baryons become bound into mid-size nuclei having less energy (and, equivalently, less mass) per nucleon compared to the original small (hydrogen) and large (plutonium etc.) nuclei. Even in electron–positron annihilation, there is no net matter being destroyed, because there was zero net matter (zero total lepton number and baryon number) to begin with before the annihilation—one lepton minus one antilepton equals zero net lepton number—and this net amount matter does not change as it simply remains zero after the annihilation.[53]

In short, matter, as defined in physics, refers to baryons and leptons. The amount of matter is defined in terms of baryon and lepton number. Baryons and leptons can be created, but their creation is accompanied by antibaryons or antileptons; and they can be destroyed by annihilating them with antibaryons or antileptons. Since antibaryons/antileptons have negative baryon/lepton numbers, the overall baryon/lepton numbers are not changed, so matter is conserved. However, baryons/leptons and antibaryons/antileptons all have positive mass, so the total amount of mass is not conserved. Further, outside of natural or artificial nuclear reactions, there is almost no antimatter generally available in the universe (see baryon asymmetry and leptogenesis), so particle annihilation is rare in normal circumstances.

Dark

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Pie chart showing the fractions of energy in the universe contributed by different sources. Ordinary matter is divided into luminous matter (the stars and luminous gases and 0.005% radiation) and nonluminous matter (intergalactic gas and about 0.1% neutrinos and 0.04% supermassive black holes). Ordinary matter is uncommon. Modeled after Ostriker and Steinhardt.[54] For more information, see NASA.
  1. Dark energy (73.0%)
  2. Dark matter (23.0%)
  3. Non-luminous matter (3.60%)
  4. Luminous matter (0.40%)

Ordinary matter, in the quarks and leptons definition, constitutes about 4% of the energy of the observable universe. The remaining energy is theorized to be due to exotic forms, of which 23% is dark matter[55][56] and 73% is dark energy.[57][58]

Galaxy rotation curve for the Milky Way. Vertical axis is speed of rotation about the galactic center. Horizontal axis is distance from the galactic center. The sun is marked with a yellow ball. The observed curve of speed of rotation is blue. The predicted curve based upon stellar mass and gas in the Milky Way is red. The difference is due to dark matter or perhaps a modification of the law of gravity.[59][60][61] Scatter in observations is indicated roughly by gray bars.

In astrophysics and cosmology, dark matter is matter of unknown composition that does not emit or reflect enough electromagnetic radiation to be observed directly, but whose presence can be inferred from gravitational effects on visible matter.[62][63] Observational evidence of the early universe and the Big Bang theory require that this matter have energy and mass, but not be composed of ordinary baryons (protons and neutrons). The commonly accepted view is that most of the dark matter is non-baryonic in nature.[62] As such, it is composed of particles as yet unobserved in the laboratory. Perhaps they are supersymmetric particles,[64] which are not Standard Model particles but relics formed at very high energies in the early phase of the universe and still floating about.[62]

Energy

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In cosmology, dark energy is the name given to the source of the repelling influence that is accelerating the rate of expansion of the universe. Its precise nature is currently a mystery, although its effects can reasonably be modeled by assigning matter-like properties such as energy density and pressure to the vacuum itself.[65][66]

Fully 70% of the matter density in the universe appears to be in the form of dark energy. Twenty-six percent is dark matter. Only 4% is ordinary matter. So less than 1 part in 20 is made out of matter we have observed experimentally or described in the standard model of particle physics. Of the other 96%, apart from the properties just mentioned, we know absolutely nothing.

— Lee Smolin (2007), The Trouble with Physics, p. 16

Exotic

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Exotic matter is a concept of particle physics, which may include dark matter and dark energy but goes further to include any hypothetical material that violates one or more of the properties of known forms of matter. Some such materials might possess hypothetical properties like negative mass.

Historical and philosophical study

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The modern conception of matter has been refined many times in history, in light of the improvement in knowledge of just what the basic building blocks are, and in how they interact. The term "matter" is used throughout physics in a wide variety of contexts: for example, one refers to "condensed matter physics",[67] "elementary matter",[68] "partonic" matter, "dark" matter, "anti"-matter, "strange" matter, and "nuclear" matter. In discussions of matter and antimatter, the former has been referred to by Alfvén as koinomatter (Gk. common matter).[69] In physics, there is no broad consensus as to a general definition of matter, and the term "matter" usually is used in conjunction with a specifying modifier.

The history of the concept of matter is a history of the fundamental length scales used to define matter. Different building blocks apply depending upon whether one defines matter on an atomic or elementary particle level. One may use a definition that matter is atoms, or that matter is hadrons, or that matter is leptons and quarks depending upon the scale at which one wishes to define matter.[70]

Classical antiquity

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In ancient India, the Buddhist, Hindu, and Jain philosophical traditions each posited that matter was made of atoms (paramanu, pudgala) that were "eternal, indestructible, without parts, and innumerable" and which associated or dissociated to form more complex matter according to the laws of nature.[6] They coupled their ideas of soul, or lack thereof, into their theory of matter. The strongest developers and defenders of this theory were the Nyaya-Vaisheshika school, with the ideas of the Indian philosopher Kanada being the most followed.[6][7] Buddhist philosophers also developed these ideas in late 1st-millennium CE, ideas that were similar to the Vaisheshika school, but ones that did not include any soul or conscience.[6] Jain philosophers included the soul (jiva), adding qualities such as taste, smell, touch, and color to each atom.[71] They extended the ideas found in early literature of the Hindus and Buddhists by adding that atoms are either humid or dry, and this quality cements matter. They also proposed the possibility that atoms combine because of the attraction of opposites, and the soul attaches to these atoms, transforms with karma residue, and transmigrates with each rebirth.[6]

In ancient Greece, pre-Socratic philosophers speculated the underlying nature of the visible world. Thales (c. 624 BCE–c. 546 BCE) regarded water as the fundamental material of the world. Anaximander (c. 610 BCE–c. 546 BCE) posited that the basic material was wholly characterless or limitless: the Infinite (apeiron). Anaximenes (flourished 585 BCE, d. 528 BCE) posited that the basic stuff was pneuma or air. Heraclitus (c. 535 BCE–c. 475 BCE) seems to say the basic element is fire, though perhaps he means that all is change. Empedocles (c. 490–430 BCE) spoke of four elements of which everything was made: earth, water, air, and fire.[72] Meanwhile, Parmenides argued that change does not exist, and Democritus argued that everything is composed of minuscule, inert bodies of all shapes called atoms, a philosophy called atomism. All of these notions had deep philosophical problems.[73]

Aristotle (384 BCE–322 BCE) was the first to put the conception on a sound philosophical basis, which he did in his natural philosophy, especially in Physics book I.[74] He adopted as reasonable suppositions the four Empedoclean elements, but added a fifth, aether. Nevertheless, these elements are not basic in Aristotle's mind. Rather they, like everything else in the visible world, are composed of the basic principles matter and form.

For my definition of matter is just this—the primary substratum of each thing, from which it comes to be without qualification, and which persists in the result.

— Aristotle, Physics I:9:192a32

The word Aristotle uses for matter, ὕλη (hyle or hule), can be literally translated as wood or timber, that is, "raw material" for building.[75] Indeed, Aristotle's conception of matter is intrinsically linked to something being made or composed. In other words, in contrast to the early modern conception of matter as simply occupying space, matter for Aristotle is definitionally linked to process or change: matter is what underlies a change of substance. For example, a horse eats grass: the horse changes the grass into itself; the grass as such does not persist in the horse, but some aspect of it—its matter—does. The matter is not specifically described (e.g., as atoms), but consists of whatever persists in the change of substance from grass to horse. Matter in this understanding does not exist independently (i.e., as a substance), but exists interdependently (i.e., as a "principle") with form and only insofar as it underlies change. It can be helpful to conceive of the relationship of matter and form as very similar to that between parts and whole. For Aristotle, matter as such can only receive actuality from form; it has no activity or actuality in itself, similar to the way that parts as such only have their existence in a whole (otherwise they would be independent wholes).

Age of Enlightenment

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French philosopher René Descartes (1596–1650) originated the modern conception of matter. He was primarily a geometer. Unlike Aristotle, who deduced the existence of matter from the physical reality of change, Descartes arbitrarily postulated matter to be an abstract, mathematical substance that occupies space:

So, extension in length, breadth, and depth, constitutes the nature of bodily substance; and thought constitutes the nature of thinking substance. And everything else attributable to body presupposes extension, and is only a mode of an extended thing.

— René Descartes, Principles of Philosophy[76]

For Descartes, matter has only the property of extension, so its only activity aside from locomotion is to exclude other bodies:[77] this is the mechanical philosophy. Descartes makes an absolute distinction between mind, which he defines as unextended, thinking substance, and matter, which he defines as unthinking, extended substance.[78] They are independent things. In contrast, Aristotle defines matter and the formal/forming principle as complementary principles that together compose one independent thing (substance). In short, Aristotle defines matter (roughly speaking) as what things are actually made of (with a potential independent existence), but Descartes elevates matter to an actual independent thing in itself.

The continuity and difference between Descartes's and Aristotle's conceptions is noteworthy. In both conceptions, matter is passive or inert. In the respective conceptions matter has different relationships to intelligence. For Aristotle, matter and intelligence (form) exist together in an interdependent relationship, whereas for Descartes, matter and intelligence (mind) are definitionally opposed, independent substances.[79]

Descartes's justification for restricting the inherent qualities of matter to extension is its permanence, but his real criterion is not permanence (which equally applied to color and resistance), but his desire to use geometry to explain all material properties.[80] Like Descartes, Hobbes, Boyle, and Locke argued that the inherent properties of bodies were limited to extension, and that so-called secondary qualities, like color, were only products of human perception.[81]

English philosopher Isaac Newton (1643–1727) inherited Descartes's mechanical conception of matter. In the third of his "Rules of Reasoning in Philosophy", Newton lists the universal qualities of matter as "extension, hardness, impenetrability, mobility, and inertia".[82] Similarly in Optics he conjectures that God created matter as "solid, massy, hard, impenetrable, movable particles", which were "...even so very hard as never to wear or break in pieces".[83] The "primary" properties of matter were amenable to mathematical description, unlike "secondary" qualities such as color or taste. Like Descartes, Newton rejected the essential nature of secondary qualities.[84]

Newton developed Descartes's notion of matter by restoring to matter intrinsic properties in addition to extension (at least on a limited basis), such as mass. Newton's use of gravitational force, which worked "at a distance", effectively repudiated Descartes's mechanics, in which interactions happened exclusively by contact.[85]

Though Newton's gravity would seem to be a power of bodies, Newton himself did not admit it to be an essential property of matter. Carrying the logic forward more consistently, Joseph Priestley (1733–1804) argued that corporeal properties transcend contact mechanics: chemical properties require the capacity for attraction.[85] He argued matter has other inherent powers besides the so-called primary qualities of Descartes, et al.[86]

19th and 20th centuries

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Since Priestley's time, there has been a massive expansion in knowledge of the constituents of the material world (viz., molecules, atoms, subatomic particles). In the 19th century, following the development of the periodic table, and of atomic theory, atoms were seen as being the fundamental constituents of matter; atoms formed molecules and compounds.[87]

The common definition in terms of occupying space and having mass is in contrast with most physical and chemical definitions of matter, which rely instead upon its structure and upon attributes not necessarily related to volume and mass. At the turn of the nineteenth century, the knowledge of matter began a rapid evolution.

Aspects of the Newtonian view still held sway. James Clerk Maxwell discussed matter in his work Matter and Motion.[88] He carefully separates "matter" from space and time, and defines it in terms of the object referred to in Newton's first law of motion.

However, the Newtonian picture was not the whole story. In the 19th century, the term "matter" was actively discussed by a host of scientists and philosophers, and a brief outline can be found in Levere.[89][further explanation needed] One textbook discussion from 1870 suggests that matter is what is made up of atoms:[90]

Three divisions of matter are recognized in science: masses, molecules and atoms.
A Mass of matter is any portion of matter appreciable by the senses.
A Molecule is the smallest particle of matter into which a body can be divided without losing its identity.
An Atom is a still smaller particle produced by division of a molecule.

Rather than simply having the attributes of mass and occupying space, matter was held to have chemical and electrical properties. In 1909 the famous physicist J. J. Thomson (1856–1940) wrote about the "constitution of matter" and was concerned with the possible connection between matter and electrical charge.[91]

In the late 19th century with the discovery of the electron, and in the early 20th century, with the Geiger–Marsden experiment discovery of the atomic nucleus, and the birth of particle physics, matter was seen as made up of electrons, protons and neutrons interacting to form atoms. There then developed an entire literature concerning the "structure of matter", ranging from the "electrical structure" in the early 20th century,[92] to the more recent "quark structure of matter", introduced as early as 1992 by Jacob with the remark: "Understanding the quark structure of matter has been one of the most important advances in contemporary physics."[93][further explanation needed] In this connection, physicists speak of matter fields, and speak of particles as "quantum excitations of a mode of the matter field".[9][10] And here is a quote from de Sabbata and Gasperini: "With the word 'matter' we denote, in this context, the sources of the interactions, that is spinor fields (like quarks and leptons), which are believed to be the fundamental components of matter, or scalar fields, like the Higgs particles, which are used to introduced mass in a gauge theory (and that, however, could be composed of more fundamental fermion fields)."[94][further explanation needed]

Protons and neutrons however are not indivisible: they can be divided into quarks. And electrons are part of a particle family called leptons. Both quarks and leptons are elementary particles, and were in 2004 seen by authors of an undergraduate text as being the fundamental constituents of matter.[95]

These quarks and leptons interact through four fundamental forces: gravity, electromagnetism, weak interactions, and strong interactions. The Standard Model of particle physics is currently the best explanation for all of physics, but despite decades of efforts, gravity cannot yet be accounted for at the quantum level; it is only described by classical physics (see Quantum gravity and Graviton)[96] to the frustration of theoreticians like Stephen Hawking. Interactions between quarks and leptons are the result of an exchange of force-carrying particles such as photons between quarks and leptons.[97] The force-carrying particles are not themselves building blocks. As one consequence, mass and energy (which to our present knowledge cannot be created or destroyed) cannot always be related to matter (which can be created out of non-matter particles such as photons, or even out of pure energy, such as kinetic energy).[citation needed] Force mediators are usually not considered matter: the mediators of the electric force (photons) possess energy (see Planck relation) and the mediators of the weak force (W and Z bosons) have mass, but neither are considered matter either.[98] However, while these quanta are not considered matter, they do contribute to the total mass of atoms, subatomic particles, and all systems that contain them.[99][100]

See also

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References

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Further reading

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from Grokipedia
Matter is defined as any substance that has and occupies , distinguishing it from and other abstract concepts in physics. It forms the basis of all tangible objects in the , from subatomic particles to galaxies, and is the subject of study in fields like physics, chemistry, and . At its most fundamental level, matter is composed of atoms, which are the smallest units of elements that retain their chemical properties; each atom consists of a dense nucleus containing protons and neutrons, surrounded by a of electrons. Protons carry a positive charge equal in magnitude but opposite to that of electrons, while neutrons are electrically neutral, and the number of protons () determines the element's identity. Atoms can combine to form molecules through chemical bonds, leading to the diverse array of substances observed in nature, such as (H₂O) or (carbon atoms in a lattice). Matter exists in multiple states or phases, primarily determined by temperature, pressure, and intermolecular forces: solids have fixed shapes and volumes due to strong particle bonds; liquids flow and take the shape of their container but maintain a fixed volume; gases expand to fill their container with neither fixed shape nor volume; and plasma, the most common state in the universe (e.g., in stars), consists of ionized particles with free electrons and nuclei. These states can transition via processes like melting, boiling, or ionization, which are reversible physical changes without altering the substance's chemical composition. Key physical properties of matter include (a measure of ), , (mass per unit ), color, , melting and boiling points, , and conductivity, all of which can be observed or measured without changing the substance's identity. In contrast, chemical properties describe how matter interacts with other substances, such as flammability, reactivity with acids, or oxidation potential, leading to irreversible chemical changes that form new substances. These properties enable the of matter into elements (pure substances like oxygen), compounds (like salt, NaCl), and mixtures (homogeneous like air or heterogeneous like ). Conservation laws underpin matter's behavior: in classical chemistry, matter is neither created nor destroyed in chemical reactions (), though in nuclear reactions or via Einstein's E=mc², matter and energy are interconvertible. Ordinary baryonic matter, made of protons and neutrons, constitutes about 5% of the universe's content, with the rest dominated by (∼27%) and (∼68%), though the nature of these remains an active area of research.

Definitions and Properties

Classical Definition

In , matter is defined as any substance that possesses and occupies a finite of , making it detectable through sensory or physical interaction. This conceptualization emphasizes matter's tangible , distinguishing it from abstract or non-material entities. For instance, everyday objects such as a wooden (solid), a glass of (liquid), or the air in a room (gas) exemplify matter in its common forms, each exhibiting measurable and spatial extent. Unlike , which treats as the capacity for work or motion without inherent or volume—such as the of a moving object or maintains its identity through interactions. Key properties include , the resistance to changes in motion proportional to its , as articulated in Newton's of motion; impenetrability, whereby two portions of cannot coexist in the same spatial point simultaneously; and divisibility, allowing to be subdivided into smaller units down to atoms in early atomic models like those proposed by . These attributes underpin the mechanical behavior of in classical frameworks. Historically, the classical understanding traces back to Aristotle's hylomorphism, in which matter (hylē) represents pure potentiality—the underlying substratum capable of receiving form (morphē) to become actualized substances—without independent existence or qualities of its own. As described in Aristotle's Physics and Metaphysics, matter persists through change as the indeterminate principle that form shapes into specific entities, such as bronze as potential statue. This philosophical foundation influenced subsequent classical views, evolving toward empirical models in the Scientific Revolution. This intuitive, macroscopic perspective laid the groundwork for later refinements in quantum mechanics.

Particle Physics Definition

In , matter is understood through the lens of as being composed exclusively of fermions, which are elementary particles characterized by half-integer spin values such as 12\frac{1}{2} and that adhere to the , preventing two identical fermions from occupying the same simultaneously. This principle, a of , ensures the stability and structure of matter by dictating how fermions interact and arrange in systems like atomic orbitals. Fermions are categorized into two main families: quarks and leptons, both of which carry specific quantum numbers, including spin, charge, and, for quarks, , that define their roles in the fundamental interactions. Baryonic matter, which constitutes the ordinary matter observed in everyday phenomena, consists primarily of baryons—composite particles formed from three quarks bound together by the strong . Protons and neutrons, the key building blocks of atomic nuclei, exemplify these baryons: a proton comprises two s and one , while a consists of one and two s, with their stability arising from the confinement of quarks within color-neutral combinations. This three-quark structure distinguishes baryons from other hadrons and underpins the composition of all visible matter in the . In the of , the fundamental fermions are organized into three generations, but the first generation provides the essential constituents of stable baryonic matter. The quarks in this generation are the (with charge +23+\frac{2}{3}) and the (with charge 13-\frac{1}{3}), while the leptons include the (charge -1) and the (neutral). These particles, all fermions obeying the , form the protons, neutrons, and electrons that assemble into atoms. In stark contrast, bosons—particles with integer spin, such as photons, gluons, and W/Z bosons—mediate the electromagnetic, , and weak forces but do not contribute to the material substance of matter itself.

Relativistic and Cosmological Perspectives

In the framework of special relativity, Albert Einstein established the mass-energy equivalence principle, expressed by the equation E=mc2E = mc^2, where EE is energy, mm is rest mass, and cc is the speed of light. This relation demonstrates that matter possesses intrinsic energy equivalent to its mass, blurring the classical distinction between the two and allowing matter to convert into other forms of energy under certain conditions. Extending to general relativity, matter's energy content, including its rest , contributes to the stress-energy tensor TμνT_{\mu\nu}, which sources the curvature of via Einstein's field equations Gμν=8πGc4TμνG_{\mu\nu} = \frac{8\pi G}{c^4} T_{\mu\nu}. The stress-energy tensor encapsulates the distribution of , , , and stress within matter fields, dictating how they influence gravitational fields and geodesic motion. Consequently, concentrations of matter, such as stars or galaxies, curve , manifesting as the gravitational attraction observed in the . In cosmology, matter plays a central role in the universe's composition and evolution within the Lambda cold dark matter (ΛCDM) model. As of 2024, observations indicate that ordinary (baryonic) matter constitutes approximately 5% of the total energy density, while accounts for about 27%, yielding a total matter fraction of roughly 32%. These proportions are derived from measurements of the and , with the total matter density parameter Ωm0.315\Omega_m \approx 0.315. The remaining ~68% is attributed to , which drives the accelerated expansion. The early transitioned through distinct eras dominated by radiation and matter following the . During the radiation-dominated era, the was governed by relativistic particles and photons, but matter domination began around 51,000 years after the , when the matter density surpassed that of radiation at z3400z \approx 3400. This shift marked a pivotal point in cosmic expansion, slowing the rate compared to the prior era and enabling the growth of large-scale structures through gravitational instability.

Composition and Structure

Atomic and Molecular Level

Matter at the atomic and molecular level consists of atoms, which serve as the fundamental building blocks of all ordinary matter. Each atom comprises a dense central nucleus containing protons—positively charged particles—and neutrons, which are electrically neutral and contribute to the atom's . Surrounding the nucleus are electrons, negatively charged particles that occupy probabilistic orbitals, determining the atom's chemical through their arrangement and interactions. The number of protons defines the element, while the balance between protons and electrons maintains electrical neutrality in isolated atoms. The periodic table organizes all known chemical elements based on increasing , which is the count of protons in the nucleus and uniquely identifies each element. This classification reveals in chemical properties, such as reactivity and valence, arising from the configurations in outer shells; for instance, elements in the same group exhibit similar bonding tendencies due to comparable numbers of valence . These patterns enable predictions of how elements combine to form compounds, underpinning chemistry's foundational principles. Isotopes are variants of the same element with identical atomic numbers but differing numbers of neutrons, affecting without altering chemical properties. isotopes, like with six protons and six neutrons, do not undergo and thus contribute to the long-term stability of matter in biological and geological systems. In contrast, unstable isotopes such as , with six protons and eight neutrons, decay over time, releasing radiation and playing roles in processes like , though they represent a minor fraction in natural matter. At the molecular level, atoms combine through chemical bonds to form s, exhibiting emergent properties distinct from individual atoms. Covalent bonds involve the sharing of electron pairs between atoms, as in diatomic oxygen (O₂), fostering strong, directional connections in nonmetals. Ionic bonds result from the electrostatic attraction between oppositely charged ions, typically formed by from metals to nonmetals, yielding crystalline solids like (NaCl). Metallic bonds feature delocalized s shared among metal atoms, enabling high electrical conductivity and malleability in substances like . A key example is (H₂O), where polar covalent bonds between oxygen and atoms create a molecule with partial charges—oxygen slightly negative and hydrogens positive—due to oxygen's higher , leading to unique properties like hydrogen bonding and solvent capabilities.

Subatomic Particles

Subatomic particles are the fundamental building blocks of atoms, consisting primarily of protons, neutrons, and , which together determine the structure and properties of matter. These particles interact through fundamental forces to form stable atomic nuclei and electron clouds, enabling the formation of elements and compounds. Protons and neutrons reside in the nucleus, while occupy orbitals around it, with their charges and masses dictating electromagnetic interactions and nuclear stability. The proton is a positively charged with a charge of +1e+1e, where ee is the of approximately 1.602×10191.602 \times 10^{-19} C, and a of approximately 1.67×10271.67 \times 10^{-27} kg. Protons define the of an element, which corresponds to the number of protons in the nucleus and thus determines the element's chemical identity and position in the periodic table. Their positive charge repels other protons but is overcome by the strong , allowing multiple protons to coexist in the nucleus. The is an electrically neutral with a mass of approximately 1.67×10271.67 \times 10^{-27} kg, slightly greater than that of the proton. contribute to the stability of the by providing additional binding through the , which counteracts the electromagnetic repulsion between protons without adding to the positive charge. The number of neutrons can vary in isotopes of the same element, affecting nuclear stability and enabling phenomena like . The is a negatively charged with a charge of 1e-1e and a of approximately 9.11×10319.11 \times 10^{-31} kg, making it about 1/1836 the of a proton. Electrons govern chemical bonding by occupying outer orbitals and participating in electromagnetic interactions, which dictate the reactivity of atoms and the conduction of in materials. Their in electron shells determines the valence and thus the chemical properties of elements. Within the nucleus, protons and neutrons—collectively known as nucleons—are bound together by the strong , one of the four fundamental interactions, which acts at very short ranges (about 10^{-15} m) to overcome proton repulsion and maintain nuclear integrity. The weak nuclear force, another fundamental interaction, plays a role in processes like , where a transforms into a proton (or vice versa), emitting an or and altering the . Protons and neutrons themselves are composite particles made up of more fundamental quarks, though their substructure is explored in greater detail elsewhere.

Fundamental Constituents

In the Standard Model of particle physics, all ordinary matter is composed of elementary fermions known as quarks and leptons. These particles are the fundamental building blocks, with quarks participating in the strong nuclear force and leptons not. There are twelve such fermions in total, organized into three generations or families, each containing two quarks and two leptons, with masses increasing across generations. Quarks come in six flavors: up, down, charm, , top, and bottom. The first generation includes the light (mass approximately 2.2 MeV/c², +2/3) and (mass approximately 4.7 MeV/c², charge -1/3), which are stable within composite particles and constitute the protons and neutrons of atomic nuclei. The second generation features the charm quark (mass ~1.27 GeV/c², charge +2/3) and (mass ~94 MeV/c², charge -1/3), while the third includes the heavy (mass ~173 GeV/c², charge +2/3) and (mass ~4.18 GeV/c², charge -1/3); the latter two are short-lived, decaying rapidly due to their high masses. Leptons also number six: the charged electron (mass 0.511 MeV/c², charge -1), (mass 105.7 MeV/c², charge -1), and (mass 1.777 GeV/c², charge -1), paired with their neutral counterparts—the , , and (with upper mass limits of <0.0008 MeV/c² for , <0.19 MeV/c² for , and <18 MeV/c² for , all at 90% CL). Only the first-generation leptons ( and ) are stable and prevalent in ordinary matter, while the muon and tau decay into lighter particles on timescales of microseconds to femtoseconds. Neutrinos interact only via the weak force and , making them notoriously difficult to detect. The three generations exhibit a pattern of increasing mass, with only the first generation appearing stably in everyday matter due to the instability of heavier particles. Quarks, unlike leptons, carry "color charge" and are subject to color confinement: they cannot exist in isolation but are perpetually bound within color-neutral hadrons, such as baryons (e.g., protons, composed of three quarks) or mesons, through the exchange of gluons mediated by (QCD). This confinement arises from a linearly increasing potential between quarks, ensuring that attempts to separate them produce new quark-antiquark pairs instead.
GenerationQuarks (Flavor, Approx. Mass in MeV/c², Charge)Leptons (Type, Approx. Mass in MeV/c², Charge)
1Up (2.2, +2/3); Down (4.7, -1/3)Electron (0.511, -1); Electron Neutrino (<8×10^{-7}, 0)
2Charm (1273, +2/3); Strange (94, -1/3)Muon (105.7, -1); Muon Neutrino (<0.19, 0)
3Top (172600, +2/3); Bottom (4183, -1/3)Tau (1777, -1); Tau Neutrino (<18, 0)

States and Phases

Common Phases

Matter exists in several common phases under everyday conditions, primarily determined by and : , , gas, and plasma. These phases represent distinct macroscopic behaviors arising from the arrangement and motion of particles, with transitions between them occurring at specific critical points where energy input or removal alters the intermolecular forces without changing the . In the solid phase, matter maintains a fixed and due to strong intermolecular forces that hold particles in a rigid, ordered lattice structure. Particles vibrate around fixed positions, with these vibrations propagating as collective waves known as phonons, which are quantized modes of . This rigidity allows solids to resist deformation under moderate forces, as seen in materials like or metals. The liquid phase features a fixed but no definite shape, as particles are close together yet free to move past one another, enabling flow. Key properties include , which measures resistance to flow due to internal between layers of molecules, and , arising from cohesive forces that minimize surface area, causing liquids like to form droplets. Liquids conform to the shape of their container while maintaining cohesion, as exemplified by mercury or . Gases occupy the full volume and shape of their container, with particles widely spaced and moving rapidly in random directions, resulting in low density and high compressibility. Intermolecular forces are negligible at typical conditions, leading to behavior approximated by the ideal gas law, expressed as PV=nRTPV = nRT where PP is pressure, VV is volume, nn is the number of moles, RR is the gas constant, and TT is temperature; this equation holds well for dilute gases like air or helium under moderate pressures and temperatures. Plasma, often considered the fourth common phase, is a partially ionized gas consisting of free electrons, ions, and neutral atoms, making it electrically conductive and responsive to electromagnetic fields. It forms at high temperatures or low pressures where sufficient energy strips electrons from atoms, as in the interiors of or discharges. Unlike neutral gases, plasmas exhibit collective behaviors like shielding and can generate magnetic fields through particle motion. Phase transitions between these states are driven by changes in or and involve s—the absorbed or released per unit without altering . transitions a to a by overcoming lattice bonds at the , requiring the of fusion, such as 334 J/g for . converts a to gas at the , absorbing the of vaporization, like 2260 J/g for , to separate molecules against cohesive forces. These processes are reversible, with freezing and releasing equivalent .

Exotic Phases

Exotic phases of matter represent states achieved under extreme conditions that transcend classical thermodynamic equilibria, revealing quantum mechanical or high-energy behaviors inherent to ordinary matter constituents. These phases often require ultralow temperatures, immense pressures, or relativistic energies to manifest, providing insights into quantum coherence, collective excitations, and fundamental interactions. Unlike everyday solids, liquids, gases, or plasmas, exotic phases exhibit macroscopic quantum effects or deconfined particle dynamics, bridging atomic scales with cosmological origins. The Bose-Einstein condensate (BEC) emerges when a dilute gas of bosons, such as rubidium-87 atoms, is cooled to temperatures mere nanokelvins above , causing the particles to occupy the lowest and form a coherent wavefunction. In this phase, matter-wave interference becomes observable on macroscopic scales, enabling phenomena like and atom lasers. The first BEC was experimentally realized on June 5, 1995, by a team at using evaporative cooling in a magnetic trap, marking a in quantum gas research. Fermionic condensates arise from ultracold gases of fermions, such as lithium-6 atoms, where attractive interactions near a Feshbach pair the particles into bosonic molecules that condense into a superfluid state. These paired fermions mimic Cooper pairs in superconductors, exhibiting zero-viscosity flow and gapless excitations, but at tunable interaction strengths spanning the BEC-BCS crossover. The initial observation occurred in through resonant pairing in a harmonic trap, demonstrating a superfluid phase distinct from bosonic counterparts. At the opposite extreme, quark-gluon plasma (QGP) forms when quarks and gluons, normally confined within hadrons, become deconfined in a hot, dense medium reaching temperatures around 101210^{12} K, as recreated in heavy-ion collisions at accelerators like the LHC. This plasma behaves as a near-perfect with minimal , reflecting strong interactions predicted by , and mirrors conditions in the early microseconds after the . Evidence for QGP was first compellingly established in 2005 from RHIC experiments, showing collective flow and jet quenching signatures. Supercritical fluids represent an intermediate exotic state where substances exceed their critical temperature and pressure, erasing the distinction between liquid and gas phases and yielding hybrid properties like high and power. For instance, at 31°C and 73 atm dissolves organics while maintaining gas-like , useful in applications. This phase highlights and scaling laws near the critical point. Glassy states, conversely, occur in supercooled liquids that avoid crystallization, forming amorphous solids with disordered atomic arrangements and high viscosity exceeding 101210^{12} Pa·s. These non-equilibrium phases trap structural disorder, exhibiting slow relaxation dynamics akin to aging, as seen in silica glass formed by rapid quenching of molten material. Glassy states underscore the kinetic barriers to equilibrium in complex systems.

Special Types

Antimatter

Antimatter consists of antiparticles that are the charge-conjugate counterparts to ordinary matter particles, possessing identical masses but opposite electric charges and other quantum numbers such as baryon number. For instance, the positron is the antiparticle of the electron, the antiproton is the counterpart to the proton, and the antineutron corresponds to the neutron; each pair shares the same rest mass while differing in charge—the positron has +1 elementary charge compared to the electron's -1, the antiproton has -1 versus the proton's +1, and the antineutron is electrically neutral like the neutron but has opposite magnetic moment and baryon number. These antiparticles can form antiatoms, such as antihydrogen (an antiproton orbited by a positron), mirroring ordinary atomic structures. Antimatter is produced naturally or artificially through processes like pair production, where a high-energy gamma ray photon interacts with a nucleus or strong electromagnetic field, converting its energy into an electron-positron pair according to Einstein's mass-energy equivalence, E=mc2E = mc^2, with the photon's energy exceeding twice the electron rest mass energy (1.022 MeV) to conserve momentum. This process exemplifies the symmetry between matter and antimatter in quantum field theory, as the vacuum can "borrow" energy briefly to create particle-antiparticle pairs that then separate. In particle accelerators, such as those at CERN, higher-energy collisions produce antiprotons and antineutrons alongside their matter counterparts. When matter and particles collide, they undergo , converting their combined rest es entirely into , primarily in the form of photons or other particles. For example, an and annihilate to produce two gamma rays each with 0.511 MeV , while a proton-antiproton collision typically yields multiple pions (π⁺, π⁻, π⁰) carrying away about 1.88 GeV of , with the pions often decaying further into photons or muons. This efficient energy release—nearly 100% of the rest —distinguishes from ordinary matter interactions, which conserve more partially. Despite this symmetry in production and annihilation, is exceedingly rare in the , a phenomenon known as , where the matter density exceeds by roughly one part in a billion (η ≈ 6 × 10⁻¹⁰ baryons per ). This imbalance arose in the early and is attributed to charge-parity ( in weak interactions, which allows slight differences in the decay rates of particles versus antiparticles, favoring matter survival over complete annihilation. Experiments like those at LHCb, including 2025 observations of in decays, confirm such in and decays, providing evidence for the mechanism behind the 's matter dominance.

Dark Matter

Dark matter is a form of matter that does not emit, absorb, or reflect light, making it invisible to electromagnetic detection, and is inferred solely through its gravitational influence on visible matter, radiation, and the large-scale structure of the universe. It is non-baryonic, meaning it is not composed of protons and neutrons like ordinary matter, as constrained by big bang nucleosynthesis predictions that limit the baryon density to about 5% of the universe's total energy content, while observations require far more mass to explain gravitational dynamics. This non-baryonic component interacts primarily through gravity and possibly the weak nuclear force, but not electromagnetism, distinguishing it from ordinary matter. Key evidence for comes from the flat rotation curves of , where orbital velocities of stars and gas remain roughly constant at large radii rather than declining as expected under Newtonian from visible alone, implying an extended halo of unseen . Gravitational lensing in colliding clusters, such as the , further supports this by showing that the —mapped through the distortion of background —aligns with the distribution of rather than the hot intracluster gas, indicating collisionless separated from baryonic matter during the merger. Observations of (CMB) anisotropies provide additional confirmation, as the power spectrum of temperature fluctuations requires a significant non-baryonic matter component to match the acoustic peaks and damping tail seen in data from the Planck satellite. In the standard cosmological model, constitutes approximately 27% of the universe's total according to Planck 2018 measurements, with the remainder being about 5% ordinary matter and 68% . This density is derived from measurements, which constrain the parameter Ω_c h² ≈ 0.120 to high precision. The paradigm, where particles are non-relativistic at the epoch of , is essential for explaining the hierarchical buildup of cosmic structures, as it allows density perturbations to grow via gravitational instability into galaxies and clusters without excessive smoothing from free-streaming or pressure effects. Leading candidates for particles include weakly interacting massive particles (WIMPs), predicted by extensions of the with masses around 10–1000 GeV/c² and weak-scale interactions; axions, ultralight particles originally proposed to solve the strong CP problem, with masses near 10^{-5} eV/c²; and sterile neutrinos, right-handed neutrinos with masses in the keV range that mix weakly with active neutrinos. As of 2025, no direct detection of these particles has been achieved despite extensive searches using underground detectors, colliders, and astrophysical probes, which have instead tightened exclusion limits on their parameter spaces. These candidates play a crucial role in the relativistic and cosmological perspectives on matter by enabling the observed large-scale structure through gravitational clustering.

Exotic Matter

Exotic matter refers to hypothetical forms of matter that exhibit properties not observed in ordinary matter, such as or , and are often invoked in to explore solutions to and quantum field theories. These concepts challenge classical intuitions about mass, energy, and stability, potentially enabling phenomena like travel or stable shortcuts, though none have been experimentally confirmed. Unlike ordinary matter, exotic forms may violate established energy conditions, leading to unusual gravitational behaviors. Negative mass matter is a purely theoretical construct where the mass parameter has an opposite sign to that of conventional matter, resulting in counterintuitive dynamics. Under Newton's second law, F=maF = ma, an applied would cause such matter to accelerate in the direction opposite to the force, as the negative mass reverses the acceleration vector. Interactions between negative and positive could lead to "runaway motion," where the pair perpetually accelerates without bound, raising questions about and stability in gravitational systems. This idea has been explored in contexts, but no experimental exists, and its viability remains speculative. Strange matter, or strange quark matter, consists of roughly equal numbers of up, down, and in a hyperdense state that could be more stable than ordinary at extreme densities. First hypothesized by in 1984, it posits that bulk strange quark matter might be the true of baryonic matter, potentially converting into "strange stars" if a small forms in their cores. Such matter would exhibit immense , comparable to that inside , with stability arising from the balance of weak interactions among quarks. Alcock, Farhi, and Olinto further developed the structural implications for compact in 1986, suggesting observable signatures like altered cooling rates, though direct detection remains elusive. Recent observations of the PSR J0614-3329 by NICER suggest it may be a strange quark star candidate. Magnetic monopoles are hypothetical elementary particles carrying an isolated magnetic charge, analogous to s but for , which is typically dipolar in nature. Dirac's 1931 quantization condition laid the groundwork by showing monopoles could explain electric charge quantization, but their modern theoretical foundation stems from grand unified theories (GUTs), where 't Hooft and Polyakov independently demonstrated in 1974 that monopoles emerge as topological solitons in non-Abelian gauge theories with . In GUTs, these monopoles would be extremely massive, on the order of 101610^{16} GeV, and their scarcity is explained by cosmic diluting their density post-Big Bang. Searches at accelerators like the LHC continue, but none have been found. One key application of lies in constructing traversable s, which require matter violating the null energy condition of to prevent collapse. Morris and Thorne's 1988 analysis showed that a throat demands density to maintain openness, threading along its geometry to counteract gravitational attraction. Similarly, the Alcubierre , proposed in 1994, envisions a bubble where with creates a contraction ahead and expansion behind a , allowing superluminal effective speeds without local motion. Both concepts highlight the theoretical necessity of but underscore challenges like quantum inequalities limiting amounts.

Conservation and Interactions

Conservation Laws

In the Standard Model of particle physics, baryon number BB is a conserved quantum number assigned to quarks and antiquarks, with B=+1/3B = +1/3 for each quark and B=1/3B = -1/3 for each antiquark, ensuring that protons and neutrons (each composed of three quarks) carry B=+1B = +1. This conservation implies that in any interaction, the total number of baryons minus antibaryons remains constant, prohibiting processes like proton decay under Standard Model dynamics. Experimental searches for baryon number violation, such as proton decay modes, have set stringent lower limits on the proton lifetime, exceeding 103410^{34} years for key channels, consistent with conservation in the Standard Model but allowing for violations in beyond-Standard-Model theories like grand unified theories (GUTs), where heavy gauge bosons can mediate ΔB=1\Delta B = 1 processes. Lepton number LL is similarly conserved in the Standard Model, with L=+1L = +1 for leptons (electrons, muons, taus, and neutrinos) and L=1L = -1 for antileptons, maintaining the balance in interactions involving these particles. While total lepton number remains invariant, neutrino oscillations—observed experimentally and driven by nonzero neutrino masses and flavor mixing—violate individual lepton flavor numbers (e.g., electron, muon, tau) but preserve the total LL. In extensions allowing Majorana neutrinos, ΔL=2\Delta L = 2 processes like neutrinoless double-beta decay could occur, though current limits exceed 102610^{26} years, supporting approximate conservation. The conservation of total matter-energy in closed systems arises from Noether's first theorem, which links continuous symmetries of the laws of physics to conserved quantities; specifically, time-translation invariance of the Lagrangian implies the (or the Hamiltonian in ). In , this extends to the conservation of the energy-momentum four-vector, ensuring that the total , including contributions from and fields, remains invariant in isolated systems. This principle underpins the equivalence of and via E=mc2E = mc^2, where matter can convert to energy (and vice versa) without altering the total. An apparent exception to strict baryon number conservation occurs in the early universe during baryogenesis, where processes involving , violation, and out-of-equilibrium conditions generated a small net excess of baryons over antibaryons (observed as the cosmic parameter η6×1010\eta \approx 6 \times 10^{-10}). Such mechanisms, potentially realized in GUTs or electroweak-scale processes like leptogenesis followed by transitions, explain why the is predominantly matter rather than annihilating into .

Role in Fundamental Forces

Matter interacts through the four fundamental forces—gravitational, electromagnetic, weak nuclear, and strong nuclear—which govern its behavior across scales from subatomic particles to galaxies. These forces arise from the exchange of force-carrying particles, or bosons, and dictate how constituents of matter, such as quarks and leptons, couple and influence physical phenomena. While the first three are described within the framework of the of , gravity remains outside it, treated separately in . The electromagnetic force acts exclusively on charged particles, including electrons, protons, and other charged hadrons, mediating their interactions via the exchange of massless photons. This force, formalized in , is responsible for everyday phenomena such as atomic structure, where electrons orbit nuclei due to attraction with protons; chemical bonding through electron sharing; and the propagation of as electromagnetic waves interacting with matter. Its infinite range and inverse-square dependence make it dominant in atomic and molecular scales, far stronger than the other forces at those distances. The weak nuclear force influences all quarks and leptons by enabling flavor-changing processes, such as the transformation of a into a proton, , and antineutrino in , which occurs in radioactive nuclei and stellar fusion. Mediated by the massive , this force operates over extremely short ranges—about 10^{-18} meters—due to the bosons' high mass, around 80-91 GeV/c², acquired through the . It underlies key astrophysical processes, like the synthesis of elements in stars, but is much weaker than except in high-energy environments. The strong nuclear force, governed by quantum chromodynamics (QCD), binds quarks—carriers of —into composite particles called hadrons, such as protons (two up quarks and one ) and neutrons (one up and two s), via the exchange of gluons. These gluons themselves carry , leading to a phenomenon called confinement, where quarks are never observed in isolation. At larger scales, the residual strong force binds protons and neutrons into atomic nuclei, overcoming electromagnetic repulsion, and is responsible for nuclear stability. Confined to nuclear dimensions (about 10^{-15} meters), it is the strongest force, approximately 100 times stronger than at short ranges. Gravity provides a universal attraction between any two objects with or , acting on all matter particles proportionally to their and over infinite distances with an . Described classically by Einstein's as the curvature of caused by mass-energy, it is negligible at subatomic scales but cumulative, dominating the motion of , , and galaxies. Unlike the other forces, its quantum description remains elusive, with the hypothetical massless proposed as the mediator, though unobserved. Gravity's weakness—about 10^{40} times feebler than the strong force—arises from its universal coupling but becomes apparent in large aggregates of matter.

Historical Development

Ancient and Medieval Views

In , the Presocratic philosophers initiated systematic inquiries into the nature of matter, seeking a unifying or archē behind the observable world. (c. 624–546 BCE) proposed as the fundamental substance, from which all things arise through processes of and , attributing to it both nutritive and generative properties essential for life and change. His successor, of Miletus (c. 610–546 BCE), advanced a more abstract view with the , an indefinite, eternal, and boundless that serves as the source of all opposites—such as hot and cold, wet and dry—encompassing and governing the without being limited to any specific observable element. Later, Democritus of Abdera (c. 460–370 BCE), building on , developed , asserting that matter consists of innumerable indivisible particles called atomos (uncuttable), differing only in shape, size, and arrangement, eternally moving through the void; sensible qualities emerge from their configurations, eliminating the need for coming-to-be or perishing from nothing. Aristotle (384–322 BCE) provided a comprehensive framework that dominated Western thought for centuries, integrating and critiquing earlier ideas through his doctrine of the four elements—earth (cold and dry), water (cold and wet), air (hot and wet), and fire (hot and dry)—which compose all terrestrial matter and transform into one another by altering their qualitative pairs. He introduced a fifth element, quintessence or aether, as the imperishable substance of the heavens, unchangeable and moving in perfect circles. Central to his ontology was hylomorphism, the theory that every physical substance is a composite of matter (hylē), the indeterminate potential substrate, and form (eidos or morphē), the actualizing principle that imparts essence, structure, and purpose; change occurs as matter receives new forms while retaining continuity. Parallel developments occurred in ancient , where the Nyaya-Vaisheshika schools (from c. 6th century BCE onward) articulated an atomic theory independent of Greek influences, positing eternal, partless atoms (paramāṇu) of four types—earth, water, air, and —as the ultimate material constituents, each inheriting perceptible qualities like color, , and touch from their inherent natures. These atoms combine in dyads and triads to form perceptible composites, with motion and aggregation governed by an inherent directional force (adṛṣṭa) and divine will, emphasizing a realist pluralism that explains diversity without a single underlying continuum. In contrast, Buddhist traditions, particularly in the texts (c. BCE–5th century CE), rejected enduring substances altogether, viewing matter as impermanent (anicca) aggregates of momentary dharmas or events—fleeting particles of physicality—that arise and cease in instantaneous flux, denying any persistent self or essence to composites and focusing on to underpin doctrines of no-self (anātman). Medieval alchemy, spanning Islamic and European contexts from the 8th to 14th centuries, adapted Aristotelian to practical pursuits, particularly the transmutation of base metals into gold and the creation of elixirs for longevity, often blending , , and proto-chemistry. In the Islamic world, (c. 721–815 CE), known as Geber, systematized these ideas in over 100 attributed treatises, expanding the four elements into a sulfur-mercury where metals form from varying proportions of volatile mercury (spirit) and fixed (body), enabling transmutation through balance and purification processes like and to reveal hidden potentials. European alchemists, influenced by Latin translations of Jabir's works via and around the 12th century, preserved and elaborated the framework; (c. 1219–1292 CE), in his Opus Maius and Speculum Alchemiae, advocated as an experimental science within , affirming the four elements as active potencies in generation and corruption, and defending transmutation as achievable through imitating nature's hidden forces, though requiring empirical verification to distinguish true from speculation. These traditions emphasized matter's transformability, laying groundwork for later chemical insights while rooted in qualitative and symbolic interpretations of the elements.

Enlightenment and Classical Physics

During the Enlightenment, advanced a mechanistic view of matter in his seminal work (1704), proposing that all matter consists of hard, impenetrable, and mobile corpuscles—tiny particles that interact through attractive and repulsive forces to form the diverse structures observed in nature. These corpuscles were envisioned as the fundamental building blocks, with their motions and attractions explaining phenomena such as cohesion, chemical affinities, and the elasticity of bodies, thereby shifting philosophical speculation toward a particle-based model grounded in observable . Building on experimental chemistry, formalized the law of in his Traité élémentaire de chimie (1789), asserting that in chemical reactions, matter is neither created nor destroyed but merely rearranged, as demonstrated through precise weighings of reactants and products in and processes. This principle, derived from quantitative experiments like the of metals, refuted earlier phlogiston theories and established mass as an invariant property, enabling the development of balanced chemical equations and stoichiometric analysis. John Dalton revived and refined atomic theory in A New System of Chemical Philosophy (), postulating that each element consists of identical, indivisible atoms differing in mass from those of other elements, and that chemical compounds form when atoms combine in simple, fixed numerical ratios by weight. Dalton's model explained the laws of definite and multiple proportions through examples like (one oxygen atom to two atoms) and supported his relative atomic weights, such as at 1 and oxygen at 7, laying the groundwork for modern chemical understanding without invoking subatomic structure. In the realm of thermodynamics during the 19th century, James Clerk Maxwell and Ludwig Boltzmann developed the kinetic theory of gases, modeling matter as collections of molecules in constant, random motion whose average kinetic energy determines temperature and pressure. Maxwell's 1860 paper derived the velocity distribution of gas molecules, showing that pressure arises from molecular collisions with container walls, while Boltzmann extended this in works like Lectures on Gas Theory (1896) by introducing the Boltzmann equation to describe how collisions redistribute energies, linking microscopic motions to macroscopic properties such as viscosity and diffusion. Rudolf Clausius contributed to the understanding of phases by formulating the Clausius-Clapeyron equation in his thermodynamic studies, which relates the pressure and temperature dependencies during phase transitions, such as liquid to vapor, by equating latent heat to changes in molecular volume and energy. This framework explained equilibrium between phases of matter, like the coexistence of ice, water, and vapor, through the second law of thermodynamics, emphasizing irreversible processes and entropy increase in heat transfers.

Modern and Contemporary Advances

The early marked a pivotal shift in understanding matter through experimental and theoretical breakthroughs in atomic structure. In 1911, Ernest Rutherford's gold foil experiment demonstrated that atoms consist of a dense, positively charged nucleus surrounded by mostly empty space, overturning the and laying the foundation for . This discovery was soon refined by in 1913, who proposed a model where electrons the nucleus in discrete energy levels, incorporating early quantum ideas to explain atomic spectra and stability. The 1920s saw the full emergence of , revolutionizing the conception of matter at microscopic scales. Werner Heisenberg's in 1925 introduced non-commuting operators to describe particle properties, resolving classical inconsistencies in atomic behavior. Complementing this, Erwin Schrödinger's 1926 provided a differential framework treating matter as wave functions, enabling probabilistic predictions of electron positions and energies in atoms. These formulations unified the quantum description of matter, influencing all subsequent developments. The mid-20th century advanced toward the of , which classifies all known matter particles. In 1964, and independently proposed quarks as fundamental constituents of protons and neutrons, explaining diversity through three quark flavors and . Leptons, including electrons and neutrinos, form another matter category, with their interactions mediated by gauge bosons as detailed in the electroweak theory developed in the 1960s and 1970s. The model's completeness was confirmed in 2012 with the discovery of the at CERN's (LHC), which imparts mass to quarks and leptons via the Higgs field, as observed by the ATLAS and CMS collaborations. Integrating relativity with quantum insights further illuminated matter's behavior in extreme conditions. Albert Einstein's 1915 general predicts that matter warps , leading to black holes where immense densities collapse stars beyond event horizons, as first theoretically described in the 1930s. In cosmology, (BBN) explains the primordial abundance of light elements like and , formed from quark-gluon plasma in the universe's first minutes, consistent with observations and parameters. Contemporary advances since the late have probed matter's subtler aspects, though fundamental revisions remain elusive as of 2025. The 1998 Super-Kamiokande experiment provided evidence for oscillations, implying non-zero masses for these leptons and extending the , with atmospheric data showing deficit consistent with mixing. Ongoing LHC searches for candidates, such as weakly interacting massive particles (WIMPs), have yielded null results through 2025, constraining models but revealing no new matter particles despite high-luminosity upgrades. No major breakthroughs in matter's core fundamentals emerged in 2024-2025, with efforts focusing on precision measurements and theoretical refinements.

References

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