Share on Facebook Share on Twitter Email
Answers.com

matter

 
(măt'ər) pronunciation
n.
    1. Something that occupies space and can be perceived by one or more senses; a physical body, a physical substance, or the universe as a whole.
    2. Physics. Something that has mass and exists as a solid, liquid, gas, or plasma.
  1. A specific type of substance: inorganic matter.
  2. Discharge or waste, such as pus or feces, from a living organism.
  3. Philosophy. In Aristotelian and Scholastic use, that which is in itself undifferentiated and formless and which, as the subject of change and development, receives form and becomes substance.
  4. The substance of thought or expression as opposed to the manner in which it is stated or conveyed.
  5. A subject of concern, feeling, or action: matters of foreign policy; a personal matter. See synonyms at subject.
  6. Trouble or difficulty: What's the matter with your car?
  7. An approximated quantity, amount, or extent: The construction will last a matter of years.
  8. Something printed or otherwise set down in writing: reading matter.
  9. Something sent by mail.
  10. Printing.
    1. Composed type.
    2. Material to be set in type.
intr.v., -tered, -ter·ing, -ters.
To be of importance: "Love is most nearly itself/When here and now cease to matter" (T.S. Eliot). See synonyms at count1.

idioms:

as a matter of fact

  1. In fact; actually.
for that matter
  1. So far as that is concerned; as for that.
no matter
  1. Regardless of: "Yet there isn't a train I wouldn't take,/No matter where it's going" (Edna St. Vincent Millay).

[Middle English, from Old French matere, from Latin māteria, wood, timber, matter, from māter, mother (because the woody part was seen as the source of growth).]


Search unanswered questions...
Enter a question here...
Search: All sources Community Q&A Reference topics

Material substance that constitutes the observable universe and, together with energy, forms the basis of all objective phenomena. Atoms are the basic building blocks of matter. Every physical entity can be described, physically and mathematically, in terms of interrelated quantities of mass, inertia, and gravitation. Matter in bulk occurs in several states; the most familiar are the gaseous (see gas), liquid, and solid states (plasmas, glasses, and various others are less clearly defined), each with characteristic properties. According to Albert Einstein's special theory of relativity, matter and energy are equivalent and interconvertible (see conservation law).

For more information on matter, visit Britannica.com.

A term that traditionally refers to the substance of which all bodiesR consist. Matter in classical mechanics is closely identified with mass. Modern analyses distinguish two types of mass: inertial mass, by which matter retains its state of rest or uniform rectilinear motion in the absence of external forces; and gravitational mass, by which a body exerts forces of attraction on other bodies, and by which it reacts to those forces. Expressed in appropriate units, these two properties are numerically equal—a purely experimental fact, unexplained by theory. Albert Einstein made the equality of inertial and gravitational mass a fundamental principle (principle of equivalence), as one of the two postulates of the theory of general relativity. See also Gravitation; Inertia; Mass; Relativity; Weight.

In quantum mechanics, mass is only one among many properties (quantum numbers) that a particle can have, for example, electric charge, spin, and parity. The nearest quantum-mechanical analogs of traditional matter are fermions, having half-integral values of spin. Forces are mediated by exchange of bosons, particles having integral spins. Fermions correspond to classical matter in exhibiting impenetrability (a consequence of the exclusion principle), but the correspondence is only rough. For example, fermions can also be exchanged in interactions (a photon and an electron can exchange an electron), and they also exhibit wavelike (nonlocalized) behavior. States of classical matter-particles were given by their positions and momenta, but in quantum mechanics it is impossible to assign simultaneous precise positions and momenta to particles. See also Exclusion principle; Quantum electrodynamics; Quantum mechanics; Quantum statistics.

The primary constituents of ordinary matter are baryonic, consisting of quarks. However it is possible that as much as 99% (by mass) of the matter in the universe consists of nonbaryonic “dark matter” whose nature is yet to be discovered. See also Baryon; Big bang theory; Cosmology; Inflationary universe cosmology; Quarks; Universe.


Roget's Thesaurus:

matter

Top

noun

  1. That which occupies space and can be perceived by the senses: materiality, substance. See body/spirit.
  2. That from which things are or can be made: material, stuff, substance. Idioms: grist for one's mill. See matter.
  3. What a speech, piece of writing, or artistic work is about: argument, point, subject, subject matter, text, theme, topic. See meaning.
  4. Something to be done, considered, or dealt with: affair, business, thing. See thing.

verb

    To be of significance or importance: count, import, signify, weigh. See important/unimportant.


n

Definition: significance, meaning
Antonyms: insignificance, meaninglessness

n

Definition: substance
Antonyms: nothing, nothingness, zero

That which occupies space, possessing size and shape, mass, movability, and solidity (which may be the same as impenetrability). Its nature was historically one of the great subjects of philosophy, now largely pursued through the philosophy of physics. Plato and Aristotle passed on a classification of matter into four kinds (earth, air, water, and fire) but also the view (not necessarily held by Aristotle himself) that any such division reflected a different form taken by one prime, undifferentiated matter or hylē (see materia prima). In Aristotle there is also a fifth kind of matter (quintessence) found in the celestial world, whose possessors were thereby exempt from change. This physics was replaced from the 17th century onwards by the classical conception first of corpuscles (see corpuscularianism) and then of modern atoms. In modern physics, the tidy picture of inert massy atoms on the one hand, and forces between them on the other, has entirely given way. The quantum mechanical description of fundamental particles blurs the distinction between matter and its energy, and between particles and the forces that describe their interaction. Philosophically, however, quantum mechanics leaves considerable unease of its own.

matter, anything that has mass and occupies space. Matter is sometimes called koinomatter (Gr. koinos=common) to distinguish it from antimatter, or matter composed of antiparticles.

The Properties of Matter

The general properties of matter result from its relationship with mass and space. Because of its mass, all matter has inertia (the mass being the measure of its inertia) and weight, if it is in a gravitational field (see gravitation). Because it occupies space, all matter has volume and impenetrability, since two objects cannot occupy the same space simultaneously.

The special properties of matter, on the other hand, depend on internal structure and thus differ from one form of matter, i.e., one substance, to another. Such properties include ductility, elasticity, hardness, malleability, porosity (ability to permit another substance to flow through it), and tenacity (resistance to being pulled apart).

The States of Matter

Matter is ordinarily observed in three different states, or phases (see states of matter), although scientists distinguish three additional states. Matter in the solid state has both a definite volume and a definite shape; matter in the liquid state has a definite volume but no definite shape, assuming the shape of whatever container it is placed in; matter in the gaseous state has neither a definite volume nor a definite shape and expands to fill any container. The properties of a plasma, or extremely hot, ionized gas, are sufficiently different from those of a gas at ordinary temperatures for scientists to consider them to be the fourth state of matter. So too are the properties of the Bose-Einstein and fermionic condensates, which exist only at temperatures approximating absolute zero (−273.15°C), and they are considered the fifth and sixth states of matter respectively.

Early Theories of Matter

In ancient times various theories were suggested about the nature of matter. Empedocles held that all matter is made up of four "elements"-earth, air, fire, and water. Leucippus and his pupil Democritus proposed an atomic basis of matter, believing that all matter is built up from tiny particles differing in size and shape. Anaxagoras, however, rejected any theory in which matter is viewed as composed of smaller constituents, whether atoms or elements, and held instead that matter is continuous throughout, being entirely of a single substance.

Modern Theory of Matter

The modern theory of matter dates from the work of John Dalton at the beginning of the 19th cent. The atom is considered the basic unit of any element, and atoms may combine chemically to form molecules, the molecule being the smallest unit of any substance that possesses the properties of that substance. An element in modern theory is any substance all of whose atoms are the same (i.e., have the same atomic number), while a compound is composed of different types of atoms together in molecules.

Physical and Chemical Changes

The difference between a mixture and a compound helps to illustrate the difference between a physical change and a chemical change. Different atoms may also be present together in a mixture, but in a mixture they are not bound together chemically as they are in a compound. In a physical change, such as a change of state (e.g., from solid to liquid), the substance as a whole changes, but its underlying structure remains the same; water is still composed of molecules containing two hydrogen atoms and one oxygen atom whether it is in the form of ice, liquid water, or steam. In a chemical change, however, the substance participates in a chemical reaction, with a consequent reordering of its atoms. As a result, it becomes a different substance with a different set of properties.

Many of the physical properties and much of the behavior of matter can be understood without detailed assumptions about the structure of atoms and molecules. For example, the kinetic-molecular theory of gases provides a good explanation of the nature of temperature and the basis of the various gas laws and also gives insight into the different states of matter. Substances in different states vary in the strength of the forces between their molecules, with intermolecular forces being strongest in solids and weakest in gases. The force holding like molecules together is called cohesion, while that between unlike molecules is called adhesion (see adhesion and cohesion). Among the phenomena resulting from intermolecular forces are surface tension and capillarity. An even larger number of aspects of matter can be understood when the nature and structure of the atom are taken into account. The quantum theory has provided the key to understanding the atom, and most basic problems relating to the atom have been solved.

The Relationship of Matter and Energy

The atomic theory of matter does not answer the question of the basic nature of matter. It is now known that matter and energy are intimately related. According to the law of mass-energy equivalence, developed by Albert Einstein as part of his theory of relativity, a quantity of matter of mass m possesses an intrinsic rest mass energy E given by E = mc2, where c is the speed of light. This equivalence is dramatically demonstrated in the phenomena of nuclear fission and fusion (see nuclear energy; nucleus), in which a small amount of matter is converted to a rather large amount of energy. The converse reaction, the conversion of energy to matter, has been observed frequently in the creation of many new elementary particles. The study of elementary particles has not solved the question of the nature of matter but only shifted it to a smaller scale.

Bibliography

See V. H. Booth, Elements of Physical Science: The Nature of Matter and Energy (1970); G. Amaldi, The Nature of Matter: Physical Theory from Thales to Fermi (1982).


The substantial facts upon which a claim or defense is based, 101 So. 2d 408, 410; the subject of litigation, upon which issue is brought before the court and joined. 368 F. 2d 648, 654.
The distinction between mind and matter is as old as philosophy and as controversial. Both are ultimately mysterious. On the view known as dualism (developed by Descartes), matter has spatial extension and non-mental properties such as divisibility, while mind is not extended in space and does not obey the laws of physics. According to the idealism of Berkeley, the notion of matter existing independently of mind is incoherent. As physics has advanced, its accounts of matter have grown even further from the 'common-sense' knowledge given by perception. This has given rise to 'two worlds' of physical reality and perceived experience. With this development matter seems to be more and more different from mind, whereas in mythology and early science mind and matter are hardly separated, and matter is seen as alive and intelligent. See also mind and body.

(Published 1987)

Word Tutor:

matter

Top
pronunciation

IN BRIEF: That which has mass and occupies space.

pronunciation The foundations of a person are not in matter but in spirit. — Ralph Waldo Emerson (1803-1882), American transcendentalist philosopher, essayist and lecturer.

LearnThatWord.com is a free vocabulary and spelling program where you only pay for results!

In physics, something that has mass and is distinct from energy. (See phases of matter.)

1. physical material having form and weight under ordinary conditions of gravity.
2. pus.

  • gray m. — matter of the central nervous system, which represents the aggregations of the nerve cells.
  • white m. — matter of the central nervous system, which comprises the axons of the nerve cells.
Random House Word Menu:

categories related to 'matter'

Top
Random House Word Menu by Stephen Glazier
For a list of words related to matter, see:

  See crossword solutions for the clue Matter.

Matter is a general term for the substance of which all physical objects consist.[1][2] Typically, matter includes atoms and other particles which have mass. A common way of defining matter is anything that has mass and volume. Mass is the amount of matter in an object and volume is the amount of space occupied by an object.[3] However, different fields use the term in different and sometimes incompatible ways; there is no single agreed scientific meaning of the word "matter".

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, was first put forward by the Greek philosophers Leucippus (~490 BC) and Democritus (~470–380 BC).[4] Over time an increasingly fine structure for matter was discovered: objects are made from molecules, molecules consist of atoms, which in turn consist of interacting subatomic particles like protons and electrons.[5][6]

Matter is commonly said to exist in four states (or phases): solid, liquid, gas and plasma. However, advances in experimental techniques have realized other phases, previously only theoretical constructs, such as Bose–Einstein condensates and fermionic condensates. A focus on an elementary-particle view of matter also leads to new phases of matter, such as the quark–gluon plasma.[7]

In physics and chemistry, matter exhibits both wave-like and particle-like properties, the so-called wave–particle duality.[8][9][10]

In the realm of cosmology, extensions of the term matter are invoked to include dark matter and dark energy, concepts introduced to explain some odd phenomena of the observable universe, such as the galactic rotation curve. These exotic forms of "matter" do not refer to matter as "building blocks", but rather to currently poorly understood forms of mass and energy.[11]

Contents

Historical development

Origins

The pre-Socratics were among the first recorded speculators about the underlying nature of the visible world. Thales (c. 624 BC–c. 546 BC) regarded water as the fundamental material of the world. Anaximander (c. 610 BC–c. 546 BC) posited that the basic material was wholly characterless or limitless: the Infinite (apeiron). Anaximenes (flourished 585 BC, d. 528 BC) posited that the basic stuff was pneuma or air. Heraclitus (c. 535–c. 475 BC) seems to say the basic element is fire, though perhaps he means that all is change. Empedocles (c. 490–430 BC) spoke of four elements of which everything was made: earth, water, air, and fire.[12] 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.[13]

Aristotle (384 BC – 322 BC) was the first to put the conception on a sound philosophical basis, which he did in his natural philosophy, especially in Physics book I.[14] 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.

The word Aristotle uses for matter, ὑλη (hyle or hule), can be literally translated as wood or timber, that is, "raw material" for building.[15] 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).

Early modernity

René Descartes (1596–1650) originated the modern conception of matter. He was primarily a geometer. Instead of, like Aristotle, deducing 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 which can be attributed to body presupposes extension, and is only a mode of that which is extended

René Descartes, Principles of Philosophy[16]

For Descartes, matter has only the property of extension, so its only activity aside from locomotion is to exclude other bodies[17]: 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.[18] They are independent things. In contrast, Aristotle defines matter and the formal/forming principle as complementary principles which 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' 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.[19]

Descartes' 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.[20] Like Descartes, Hobbes, Boyle, and Locke argued that the inherent propeties of bodies were limited to extension, and that so-called secondary qualities, like color, were only products of human perception.[21]

Isaac Newton (1643–1727) inherited Descartes' 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."[22] 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."[23] 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.[24]

Newton developed Descartes' 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' mechanics, in which interactions happened exclusively by contact.[25]

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 argued that corporeal properties transcend contact mechanics: chemical properties require the capacity for attraction.[25] He argued matter has other inherent powers besides the so-called primary qualities of Descartes, et al.[26]

Since Priestley's time, there has been a massive expansion in knowledge of the constituents of the material world (viz., molecules, atoms, subatomic particles), but there has been no further development in the definition of matter. Rather the question has been set aside. Noam Chomsky summarizes the situation that has prevailed since that time:

What is the concept of body that finally emerged?[...] The answer is that there is no clear and definite conception of body.[...] Rather, the material world is whatever we discover it to be, with whatever properties it must be assumed to have for the purposes of explanatory theory. Any intelligible theory that offers genuine explanations and that can be assimilated to the core notions of physics becomes part of the theory of the material world, part of our account of body. If we have such a theory in some domain, we seek to assimilate it to the core notions of physics, perhaps modifying these notions as we carry out this enterprise.

Noam Chomsky, 'Language and problems of knowledge: the Managua lectures, p. 144[25]

So matter is whatever physics studies and the object of study of physics is matter: there is no independent general definition of matter, apart from its fitting into the methodology of measurement and controlled experimentation. In sum, the boundaries between what constitutes matter and everything else remains as vague as the demarcation problem of delimiting science from everything else.[27]

Late nineteenth and early twentieth centuries

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.[28]

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.[29] 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.[30][further explanation needed] A textbook discussion from 1870 suggests matter is what is made up of atoms:[31]

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. The famous physicist J. J. Thomson wrote about the "constitution of matter" and was concerned with the possible connection between matter and electrical charge.[32]

Later developments

There is an entire literature concerning the "structure of matter", ranging from the "electrical structure" in the early 20th century,[33] to the more recent "quark structure of matter", introduced today with the remark: Understanding the quark structure of matter has been one of the most important advances in contemporary physics.[34][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".[8][9] 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 which, however, could be composed of more fundamental fermion fields)."[35][further explanation needed]

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.

In the late 19th century with the discovery of the electron, and in the early 20th century, with the 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. Today, we know that even protons and neutrons are not indivisible, they can be divided into quarks, while electrons are part of a particle family called leptons. Both quarks and leptons are elementary particles, and are currently seen as being the fundamental constituents of matter.[36]

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).[37] Interactions between quarks and leptons are the result of an exchange of force-carrying particles (such as photons) between quarks and leptons.[38] The force-carrying particles are not themselves building blocks. As one consequence, mass and energy (which 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). Force carriers are usually not considered matter: the carriers of the electric force (photons) possess energy (see Planck relation) and the carriers of the weak force (W and Z bosons) are massive, but neither are considered matter either.[39] However, while these particles are not considered matter, they do contribute to the total mass of atoms, subatomic particles, and all systems which contain them.[40][41]

Summary

The term "matter" is used throughout physics in a bewildering variety of contexts: for example, one refers to "condensed matter physics",[42] "elementary matter",[43] "partonic" matter, "dark" matter, "anti"-matter, "strange" matter, and "nuclear" matter. In discussions of matter and antimatter, normal matter has been referred to by Alfvén as koinomatter.[44] It is fair to say that 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.

Definitions

Common definition

The DNA molecule is an example of matter under the "atoms and molecules" definition.

The common definition of matter is anything that has both mass and volume (occupies space).[45][46] For example, a car would be said to be made of matter, as it occupies space, and has mass.

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 Pauli exclusion principle.[47][48] 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.

Relativity

In the context of relativity, mass is not an additive quantity.[1] Thus, in relativity usually a more general view is taken that it is not mass, but the energy–momentum tensor that quantifies the amount of matter. Matter therefore is anything that contributes to the energy–momentum of a system, that is, anything that is not purely gravity.[49][50] This view is commonly held in fields that deal with general relativity such as cosmology.

Atoms and molecules definition

A definition of "matter" that is based upon its physical and chemical structure is: matter is made up of atoms and molecules.[51] 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 and molecules definition. Alternatively, one can adopt the protons, neutrons and electrons definition.

Protons, neutrons and electrons definition

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.[52] 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 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 (see Quarks and leptons definition below).

Quarks and leptons definition

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 may be seen from the above discussion, many early definitions of what can be called ordinary matter were based upon 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 elementary fermions, namely quarks and leptons.[53][54] 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 the two types of elementary fermions. 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.[55] (Higher generations particles quickly decay into first-generation particles, and thus are not commonly encountered.[56])

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.[57] 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.[58] 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 gluons fields contribute significantly to the mass of hadrons.[59] In other words, most of what composes the "mass" of ordinary matter is due to the binding energy of quarks within protons and neutrons.[60] 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).[56][61] The bottom line is that most of the mass of everyday objects comes from the interaction energy of its elementary components.

Smaller building blocks?

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.[62] 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.[63]

Structure

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

Quarks

Quarks are 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. Quarks are massive particles, and therefore are also subject to gravity.

Quark properties[64]
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
Quark structure of a proton: 2 up quarks and 1 down quark.

Baryonic matter

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 is usually used to refer to triquarks — particles made of three quarks. "Exotic" baryons made of four quarks and one antiquark are known as the 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 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 baryionic matter. About 23% is dark matter, and about 72% is dark energy.[65]

A comparison between the white dwarf IK Pegasi B (center), its A-class companion IK Pegasi A (left) and the Sun (right). This white dwarf has a surface temperature of 35,500 K.

Degenerate matter

In physics, degenerate matter refers to the ground state of a gas of fermions at a temperature near absolute zero.[66] 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 for the case of many fermions the maximum kinetic energy called the Fermi energy and the pressure of the gas becomes very large and dependent upon 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.[67] 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.[68]

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

Strange matter

Strange matter is a particular form of quark matter, usually thought of as a 'liquid' of up, down, and strange quarks. It is to be 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 containing 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 of the term "strange matter"

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 [69] and Witten.[70] 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

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[71]
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[72]
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

Phase diagram for a typical substance at a fixed volume. Vertical axis is Pressure, horizontal axis is Temperature. The green line marks the freezing point (above the green line is solid, below it is liquid) and the blue line the boiling point (above it is liquid and below it is gas). So, for example, at higher T, a higher P is necessary to maintain the substance in liquid phase. At the triple point the three phases; liquid, gas and solid; can coexist. Above the critical point there is no detectable difference between the phases. The dotted line shows the anomalous behavior of water: ice melts at constant temperature with increasing pressure.[73]

In bulk, matter can exist in several different forms, or states of aggregation, known as phases,[74] depending on ambient pressure, temperature and volume.[75] 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

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

In particle physics and quantum chemistry, 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 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.

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 which 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, and whether other places are almost entirely antimatter 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 the charge parity (or CP symmetry) violation. CP symmetry violation can be obtained from the Standard Model,[76] 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.

Other types of matter

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.[77] For more information, see NASA.

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[78][79] and 73% is dark energy.[80][81]

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.[82][83][84] Scatter in observations is indicated roughly by gray bars.

Dark matter

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.[11][85] Observational evidence of the early universe and the big bang theory require that this matter have energy and mass, but is not composed of either elementary fermions (as above) OR gauge bosons. The commonly accepted view is that most of the dark-matter is non-baryonic in nature.[11] As such, it is composed of particles as yet unobserved in the laboratory. Perhaps they are supersymmetric particles,[86] which are not Standard Model particles, but relics formed at very high energies in the early phase of the universe and still floating about.[11]

Dark energy

In cosmology, dark energy is the name given to the antigravitating influence that is accelerating the rate of expansion of the universe. It is known not to be composed of known particles like protons, neutrons or electrons, nor of the particles of dark matter, because these all gravitate.[87][88]

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: The Trouble with Physics, p. 16

Exotic matter

Exotic matter is a hypothetical concept of particle physics. It covers any material which violates one or more classical conditions or is not made of known baryonic particles. Such materials would possess qualities like negative mass or being repelled rather than attracted by gravity.

See also

Antimatter

Cosmology

Dark matter

Philosophy

Other

References

  1. ^ a b R. Penrose (1991). "The mass of the classical vacuum". In S. Saunders, H.R. Brown. The Philosophy of Vacuum. Oxford University Press. p. 21. ISBN 0198244495. http://books.google.com/?id=ZU1LL4IbDKcC&pg=PA21. 
  2. ^ "Matter (physics)". McGraw-Hill's Access Science: Encyclopedia of Science and Technology Online. http://www.accessscience.com/abstract.aspx?id=410600&referURL=http%3a%2f%2fwww.accessscience.com%2fcontent.aspx%3fid%3d410600. Retrieved 2009-05-24. 
  3. ^ J. Mongillo (2007). Nanotechnology 101. Greenwood Publishing. p. 30. ISBN 0313338809. http://books.google.com/?id=j69lwrrQ4nsC&pg=PA30. 
  4. ^ J. Olmsted, G.M. Williams (1996). Chemistry: The Molecular Science (2nd ed.). Jones & Bartlett. p. 40. ISBN 0815184506. http://books.google.com/?id=1vnk6J8knKkC&pg=PA40. 
  5. ^ P. Davies (1992). The New Physics: A Synthesis. Cambridge University Press. p. 1. ISBN 0521438314. http://books.google.com/?id=akb2FpZSGnMC&pg=PA1. 
  6. ^ G. 't Hooft (1997). In search of the ultimate building blocks. Cambridge University Press. p. 6. ISBN 0521578833. http://books.google.com/?id=e-7eAp-bVbEC&pg=PA6. 
  7. ^ "RHIC Scientists Serve Up "Perfect" Liquid" (Press release). Brookhaven National Laboratory. 18 April 2005. http://www.bnl.gov/bnlweb/pubaf/pr/pr_display.asp?prid=05-38. Retrieved 2009-09-15. 
  8. ^ a b P.C.W. Davies (1979). The Forces of Nature. Cambridge University Press. p. 116. ISBN 052122523X. http://books.google.com/?id=Av08AAAAIAAJ&pg=PA116&dq=%22matter+field%22. 
  9. ^ a b S. Weinberg (1998). The Quantum Theory of Fields. Cambridge University Press. p. 2. ISBN 0521550025. http://books.google.com/?id=2oPZJJerMLsC&pg=PA5&dq=Weinberg+%22matter+field%22. 
  10. ^ M. Masujima (2008). Path Integral Quantization and Stochastic Quantization. Springer. p. 103. ISBN 3540878505. http://books.google.com/?id=OM15pk3ZHf0C&pg=PA103. 
  11. ^ a b c d D. Majumdar (2007). "Dark matter — possible candidates and direct detection". arXiv:hep-ph/0703310 [hep-ph]. 
  12. ^ S. Toulmin, J. Goodfield (1962). The Architecture of Matter. University of Chicago Press. pp. 48–54. 
  13. ^ Discussed by Aristotle in Physics, esp. book I, but also later; as well as Metaphysics I-II.
  14. ^ For a good explanation and elaboration, see R.J. Connell (1966). Matter and Becoming. Priory Press. 
  15. ^ H.G. Liddell, R. Scott, J.M. Whiton (1891). A lexicon abridged from Liddell & Scott's Greek-English lexicon. Harper and Brothers. p. 725. http://books.google.com/?id=nxoyBcpUuEsC&lpg=PA829&dq=liddell%20and%20scott%20hyle&pg=PA725#v=onepage&q=. 
  16. ^ R. Descartes (1644). "The Principles of Human Knowledge". Principles of Philosophy I. p. 53. 
  17. ^ though even this property seems to be non-essential (Rene Descartes, Principles of Philosophy II [1644], “On the Principles of Material Things,” no. 4.)
  18. ^ R. Descartes (1644). "The Principles of Human Knowledge". Principles of Philosophy I. pp. 8, 54, 63. 
  19. ^ D.L. Schindler (1986). "The Problem of Mechanism". In D.L. Schindler. Beyond Mechanism. University Press of America. 
  20. ^ E.A. Burtt, Metaphysical Foundations of Modern Science (Garden City, NY: Doubleday and Company, 1954), 117-118.
  21. ^ J.E. McGuire and P.M. Heimann, "The Rejection of Newton's Concept of Matter in the Eighteenth Century," The Concept of Matter in Modern Philosophy ed. Ernan McMullin (Notre Dame: University of Notre Dame Press, 1978), 104-118 (105).
  22. ^ Isaac Newton, Mathematical Principles of Natural Philosophy, trans. A. Motte, revised by F. Cajori (Berkeley: University of California Press, 1934), pp. 398-400. Further analyzed by Maurice A. Finocchiaro, "Newton's Third Rule of Philosophizing: A Role for Logic in Historiography," Isis 65:1 (Mar. 1974), pp. 66-73.
  23. ^ Isaac Newton, Optics, Book III, pt. 1, query 31.
  24. ^ McGuire and Heimann, 104.
  25. ^ a b c N. Chomsky (1988). Language and problems of knowledge: the Managua lectures (2nd ed.). MIT Press. p. 144. ISBN 0262530708. http://books.google.com/books?id=hwgHVRZtK8kC&pg=PA144. 
  26. ^ McGuire and Heimann, 113.
  27. ^ Nevertheless, it remains true that the mathematization regarded as requisite for a modern physical theory carries its own implicit notion of matter, which is very like Descartes', despite the demonstrated vacuity of the latter's notions.
  28. ^ M. Wenham (2005). Understanding Primary Science: Ideas, Concepts and Explanations (2nd ed.). Paul Chapman Educational Publishing. p. 115. ISBN 1412901634. http://books.google.com/?id=9vWrbr42VA0C&pg=PA115. 
  29. ^ J.C. Maxwell (1876). Matter and Motion. Society for Promoting Christian Knowledge. p. 18. ISBN 0486668959. http://books.google.com/?id=MWoOAAAAIAAJ&printsec=frontcover&dq=matter. 
  30. ^ T.H. Levere (1993). "Introduction". Affinity and Matter: Elements of Chemical Philosophy, 1800–1865. Taylor & Francis. ISBN 2881245838. http://books.google.com/?id=gKSDWsE8fZMC&printsec=frontcover&dq=matter. 
  31. ^ G.F. Barker (1870). "Introduction". A Text Book of Elementary Chemistry: Theoretical and Inorganic. John P. Morton and Company. p. 2. http://books.google.com/?id=B6Yz6eW-5joC. 
  32. ^ J.J. Thomson (1909). "Preface". Electricity and Matter. A. Constable. http://books.google.com/?id=2AaToepvKoEC&printsec=titlepage#PPP13,M1. 
  33. ^ O.W. Richardson (1914). "Chapter 1". The Electron Theory of Matter. The University Press. http://books.google.com/?id=RpdDAAAAIAAJ&printsec=frontcover&dq=matter. 
  34. ^ M. Jacob (1992). The Quark Structure of Matter. World Scientific. ISBN 9810236875. http://books.google.com/?id=iQ1e2a9bPikC&printsec=frontcover&dq=matter. 
  35. ^ V. de Sabbata, M. Gasperini (1985). Introduction to Gravitation. World Scientific. p. 293. ISBN 9971500493. http://books.google.com/?id=7sJ6m8s0_ccC&pg=PA293&dq=Weinberg+%22matter+field%22. 
  36. ^ 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. B. Povh, K. Rith, C. Scholz, F. Zetsche, M. Lavelle (2004). "Fundamental constituents of matter". Particles and Nuclei: An Introduction to the Physical Concepts (4th ed.). Springer. ISBN 3540201688. http://books.google.com/?id=rJe4k8tkq7sC&pg=PA9&dq=povh+%22building+blocks+of+matter%22. 
  37. ^ J. Allday (2001). Quarks, Leptons and the Big Bang. CRC Press. p. 12. ISBN 0750308060. http://books.google.com/?id=kgsBbv3-9xwC&pg=PA12. 
  38. ^ B.A. Schumm (2004). Deep Down Things: The Breathtaking Beauty of Particle Physics. Johns Hopkins University Press. p. 57. ISBN 080187971X. http://books.google.com/?id=htJbAf7xA_oC&pg=PA57. 
  39. ^ See for example, M. Jibu, K. Yasue (1995). Quantum Brain Dynamics and Consciousness. John Benjamins Publishing Company. p. 62. ISBN 1556191839. http://books.google.com/?id=iNUvcniwvg0C&pg=PA62. , B. Martin (2009). Nuclear and Particle Physics (2nd ed.). Wiley. p. 125. ISBN 0470742755. http://books.google.com/?id=ws8QZ2M5OR8C&pg=PT143.  and K.W. Plaxco, M. Gross (2006). Astrobiology: A Brief Introduction. Johns Hopkins University Press. p. 23. ISBN 0801883679. http://books.google.com/?id=2JuGDL144BEC&pg=PA23. 
  40. ^ P.A. Tipler, R.A. Llewellyn (2002). Modern Physics. Macmillan. pp. 89–91, 94–95. ISBN 0716743450. http://books.google.com/?id=tpU18JqcSNkC&pg=PA94. 
  41. ^ P. Schmüser, H. Spitzer (2002). "Particles". In L. Bergmann et al.. Constituents of Matter: Atoms, Molecules, Nuclei. CRC Press. pp. 773 ff. ISBN 0849312027. http://books.google.com/?id=mGj1y1WYflMC&printsec=frontcover#PPA773,M1. 
  42. ^ P.M. Chaikin, T.C. Lubensky (2000). Principles of Condensed Matter Physics. Cambridge University Press. p. xvii. ISBN 0521794501. http://books.google.com/?id=P9YjNjzr9OIC&printsec=frontcover&dq=matter. 
  43. ^ W. Greiner (2003). W. Greiner, M.G. Itkis, G. Reinhardt, M.C. Güçlü. ed. Structure and Dynamics of Elementary Matter. Springer. p. xii. ISBN 1402024452. http://books.google.com/?id=ORyJzhAzpUgC&printsec=frontcover&dq=matter. 
  44. ^ P. Sukys (1999). Lifting the Scientific Veil: Science Appreciation for the Nonscientist. Rowman & Littlefield. p. 87. ISBN 0847696006. http://books.google.com/?id=WEM4hqxJ-xYC&pg=PR23&dq=isbn=0847696006#PPA87,M1. 
  45. ^ S.M. Walker, A. King (2005). What is Matter?. Lerner Publications. p. 7. ISBN 0822551314. http://books.google.com/?id=o7EquxOl4MAC&printsec=frontcover&dq=matter. 
  46. ^ J.Kenkel, P.B. Kelter, D.S. Hage (2000). Chemistry: An Industry-based Introduction with CD-ROM. CRC Press. p. 2. ISBN 1566703034. http://books.google.com/?id=ADSjPRl_tgoC&pg=PA1&dq=matter+chemistry+properties. "All basic science textbooks define matter as simply the collective aggregate of all material substances that occupy space and have mass or weight." 
  47. ^ K.A. Peacock (2008). The Quantum Revolution: A Historical Perspective. Greenwood Publishing Group. p. 47. ISBN 031333448X. http://books.google.com/?id=ITqnf5jdE5QC&pg=PA47&dq=%22prevents+matter+from+collapsing%22. 
  48. ^ M.H. Krieger (1998). Constitutions of Matter: Mathematically Modeling the Most Everyday of Physical Phenomena. University of Chicago Press. p. 22. ISBN 0226453057. http://books.google.com/?id=VduHhkzl-aQC&pg=PA22&dq=%22does+not+collapse+into+itself%22. 
  49. ^ S.M. Caroll (2004). Spacetime and Geometry. Addison Wesley. pp. 163–164. ISBN 0-8053-8732-3. 
  50. ^ P. Davies (1992). The New Physics: A Synthesis. Cambridge University Press. p. 499. ISBN 0521438314. http://books.google.com/?id=akb2FpZSGnMC&pg=PA499. "Matter fields: the fields whose quanta describe the elementary particles that make up the material content of the Universe (as opposed to the gravitons and their supersymmetric partners)." 
  51. ^ G.F. Barker (1870). "Divisions of matter". A text-book of elementary chemistry: theoretical and inorganic. John F Morton & Co.. p. 2. ISBN 9781446022061. http://books.google.com/?id=az8AAAAAYAAJ&pg=PA2&dq=%22Three+divisions+of+matter+are+recognized%22&q=%22Three%20divisions%20of%20matter%20are%20recognized%22. 
  52. ^ M. de Podesta (2002). Understanding the Properties of Matter (2nd ed.). CRC Press. p. 8. ISBN 0415257883. http://books.google.com/?id=h8BNvnR050cC&pg=PA8. 
  53. ^ B. Povh, K. Rith, C. Scholz, F. Zetsche, M. Lavelle (2004). "Part I: Analysis: The building blocks of matter". Particles and Nuclei: An Introduction to the Physical Concepts (4th ed.). Springer. ISBN 3540201688. http://books.google.com/?id=rJe4k8tkq7sC&pg=PA9&dq=povh+%22building+blocks+of+matter%22. 
  54. ^ B. Carithers, P. Grannis (1995). "Discovery of the Top Quark". Beam Line (SLAC) 25 (3): 4–16. http://www.slac.stanford.edu/pubs/beamline/pdf/95iii.pdf. 
  55. ^ See p.7 in B. Carithers, P. Grannis (1995). "Discovery of the Top Quark". Beam Line (SLAC) 25 (3): 4–16. http://www.slac.stanford.edu/pubs/beamline/pdf/95iii.pdf. 
  56. ^ a b D. Green (2005). High PT physics at hadron colliders. Cambridge University Press. p. 23. ISBN 0521835097. http://books.google.com/?id=6-7TE5N0vbIC&pg=PA23. 
  57. ^ L. Smolin (2007). The Trouble with Physics: The Rise of String Theory, the Fall of a Science, and What Comes Next. Mariner Books. p. 67. ISBN 061891868X. http://books.google.com/?id=z5rxrnlcp3sC&pg=PA67&dq=%22all+the+particles+that+make+up+matter%22. 
  58. ^ The W boson mass is 80.398 GeV; see Figure 1 in C. Amsler et al. (Particle Data Group) (2008). "Review of Particle Physics: The Mass and Width of the W Boson". Physics Letters B 667: 1. Bibcode 2008PhLB..667....1P. doi:10.1016/j.physletb.2008.07.018. http://pdg.lbl.gov/2008/reviews/wmass_s043202.pdf. 
  59. ^ I.J.R. Aitchison, A.J.G. Hey (2004). Gauge Theories in Particle Physics. CRC Press. p. 48. ISBN 0750308648. http://books.google.com/?id=vLP7XN2pWlEC&pg=PA48&dq=%22source+particles+of+the+gluon+fields%22. 
  60. ^ B. Povh, K. Rith, C. Scholz, F. Zetsche, M. Lavelle (2004). Particles and Nuclei: An Introduction to the Physical Concepts. Springer. p. 103. ISBN 3540201688=. http://books.google.com/?id=rJe4k8tkq7sC&pg=PA103&dq=%22interquark+interaction+energy%22. 
  61. ^ T. Hatsuda (2008). "Quark-gluon plasma and QCD". In H. Akai. Condensed matter theories. 21. Nova Publishers. p. 296. ISBN 1600215017. http://books.google.com/?id=PZdFi145170C&pg=PA296. 
  62. ^ K.W Staley (2004). "Origins of the third generation of matter". The evidence for the top quark. Cambridge University Press. p. 8. ISBN 0521827108. http://books.google.com/?id=DLt_fcBYynAC&pg=PA8. 
  63. ^ Y. Ne'eman, Y. Kirsh (1996). The Particle Hunters (2nd ed.). Cambridge University Press. p. 276. ISBN 0521476860. http://books.google.com/?id=K4jcfCguj8YC&pg=PA276. "[T]he most natural explanation to the existence of higher generations of quarks and leptons is that they correspond to excited states of the first generation, and experience suggests that excited systems must be composite" 
  64. ^ C. Amsler et al. (Particle Data Group) (2008). "Reviews of Particle Physics: Quarks". Physics Letters B 667: 1. Bibcode 2008PhLB..667....1P. doi:10.1016/j.physletb.2008.07.018. http://pdg.lbl.gov/2008/tables/rpp2008-sum-quarks.pdf. 
  65. ^ "Five Year Results on the Oldest Light in the Universe". NASA. 2008. http://map.gsfc.nasa.gov/m_mm.html. Retrieved 2008-05-02. 
  66. ^ H.S. Goldberg, M.D. Scadron (1987). Physics of Stellar Evolution and Cosmology. Taylor & Francis. p. 202. ISBN 0677055404. http://books.google.com/?id=NowVde8kzIoC&pg=PA207&dq=matter+%22exclusion+principle%22. 
  67. ^ H.S. Goldberg, M.D. Scadron (1987). Physics of Stellar Evolution and Cosmology. Taylor & Francis. p. 233. ISBN 0677055404. http://books.google.com/?id=NowVde8kzIoC&pg=PA207&dq=matter+%22exclusion+principle%22. 
  68. ^ J.-P. Luminet, A. Bullough, A. King (1992). Black Holes. Cambridge University Press. p. 75. ISBN 0521409063. http://books.google.com/?id=WRexJODPq5AC&pg=PA72&dq=matter+%22exclusion+principle%22. 
  69. ^ A. Bodmer (1971). "Collapsed Nuclei". Physical Review D 4 (6): 1601. Bibcode 1971PhRvD...4.1601B. doi:10.1103/PhysRevD.4.1601. 
  70. ^ E. Witten (1984). "Cosmic Separation of Phases". Physical Review D 30 (2): 272. Bibcode 1984PhRvD..30..272W. doi:10.1103/PhysRevD.30.272. 
  71. ^ C. Amsler et al. (Particle Data Group) (2008). "Review of Particle Physics: Leptons". Physics Letters B 667: 1. Bibcode 2008PhLB..667....1P. doi:10.1016/j.physletb.2008.07.018. http://pdg.lbl.gov/2008/tables/rpp2008-sum-leptons.pdf. 
  72. ^ C. Amsler et al. (Particle Data Group) (2008). "Review of Particle Physics: Neutrinos Properties". Physics Letters B 667: 1. Bibcode 2008PhLB..667....1P. doi:10.1016/j.physletb.2008.07.018. http://pdg.lbl.gov/2008/listings/s066.pdf. 
  73. ^ S.R. Logan (1998). Physical Chemistry for the Biomedical Sciences. CRC Press. pp. 110–111. ISBN 0748407103. http://books.google.com/?id=LA_8QzoCNMsC&pg=PA110&dq=water+%22phase++diagram%22. 
  74. ^ P.J. Collings (2002). "Chapter 1: States of Matter". Liquid Crystals: Nature's Delicate Phase of Matter. Princeton University Press. ISBN 0691086729. http://books.google.com/?id=NE1RWiGXtdUC&printsec=frontcover#PPA1,M1. 
  75. ^ D.H. Trevena (1975). "Chapter 1.2: Changes of phase". The Liquid Phase. Taylor & Francis. ISBN 9780851090313. http://books.google.com/?id=oOkOAAAAQAAJ&pg=PA1&dq=phase+of+matter. 
  76. ^ National Research Council (US) (2006). Revealing the hidden nature of space and time. National Academies Press. p. 46. ISBN 0309101948. http://books.google.com/?id=oTedc3rTDr4C&pg=PA46. 
  77. ^ J.P. Ostriker, P.J. Steinhardt (2003). "New Light on Dark Matter". Science 300 (5627): 1909–13. arXiv:astro-ph/0306402. Bibcode 2003Sci...300.1909O. doi:10.1126/science.1085976. PMID 12817140. 
  78. ^ K. Pretzl (2004). "Dark Matter, Massive Neutrinos and Susy Particles". Structure and Dynamics of Elementary Matter. Walter Greiner. p. 289. ISBN 1402024460. http://books.google.com/?id=lokz2n-9gX0C&pg=PA289&dq=matter+%22massive+particles%22. 
  79. ^ K. Freeman, G. McNamara (2006). "What can the matter be?". In Search of Dark Matter. Birkhäuser Verlag. p. 105. ISBN 0387276165. http://books.google.com/?id=C2OS1kmQ8JIC&pg=PA45&dq=isbn=0387276165#PPA105,M1. 
  80. ^ J.C. Wheeler (2007). Cosmic Catastrophes: Exploding Stars, Black Holes, and Mapping the Universe. Cambridge University Press. p. 282. ISBN 0521857147. http://books.google.com/?id=j1ej8d0F8jAC&pg=PA282&dq=%22dark+energy%22+date:2002-2009. 
  81. ^ J. Gribbin (2007). The Origins of the Future: Ten Questions for the Next Ten Years. Yale University Press. p. 151. ISBN 0300125968. http://books.google.com/?id=f6AYrZYGig8C&pg=PA151&dq=%22dark+energy%22+date:2002-2009. 
  82. ^ P. Schneider (2006). Extragalactic Astronomy and Cosmology. Springer. p. 4, Fig. 1.4. ISBN 3540331743. http://books.google.com/?id=uP1Hz-6sHaMC&pg=PA100&dq=rotation+Milky+way. 
  83. ^ T. Koupelis, K.F. Kuhn (2007). In Quest of the Universe. Jones & Bartlett Publishers. p. 492; Fig. 16.13. ISBN 0763743879. http://books.google.com/?id=6rTttN4ZdyoC&pg=PA491&dq=Milky+Way+%22rotation+curve%22. 
  84. ^ M.H. Jones, R.J. Lambourne, D.J. Adams (2004). An Introduction to Galaxies and Cosmology. Cambridge University Press. p. 21; Fig. 1.13. ISBN 0521546230. http://books.google.com/?id=36K1PfetZegC&pg=PA20&dq=Milky+Way+%22rotation+curve%22. 
  85. ^ K.A. Olive (2003). "Theoretical Advanced Study Institute lectures on dark matter". arXiv:astro-ph/0301505 [astro-ph]. 
  86. ^ K.A. Olive (2009). "Colliders and Cosmology". European Physical Journal C 59 (2): 269–295. arXiv:0806.1208. Bibcode 2009EPJC...59..269O. doi:10.1140/epjc/s10052-008-0738-8. 
  87. ^ J.C. Wheeler (2007). Cosmic Catastrophes. Cambridge University Press. p. 282. ISBN 0521857147. http://books.google.com/?id=j1ej8d0F8jAC&pg=PA282&dq=%22dark+energy%22. 
  88. ^ L. Smolin (2007). The Trouble with Physics. Mariner Books. p. 16. ISBN 061891868X. http://books.google.com/?id=z5rxrnlcp3sC&pg=PA16. 

Further reading

External links


Translations:

Matter

Top

Dansk (Danish)
n. - sag, spørgsmål, anliggende, ting
v. intr. - betyde noget, have betydning, gøre noget

idioms:

  • a matter of    cirka, omtrent, en sag om, et spørgsmål om
  • as a matter of course    selvfølgelighed
  • as a matter of fact    faktum, kendsgerning
  • dead matter    død substans
  • for that matter    for så vidt angår
  • foul matter    aflægning (grafisk industri), snavs, noget urent
  • no matter    uanset

Nederlands (Dutch)
materie, stof, aangelegenheid, hoeveelheid, belang, probleem, omstandigheid, aanleiding, materiaal, afvalmateriaal van het lichaam, post, pus, iets uitmaken, er iets toe doen, etteren

Français (French)
n. - (gén) chose, affaire, problème, question, point, (Sci) matière, contenu (d'un livre), le fond, (Méd) pus
v. intr. - être important, avoir de l'importance, aller

idioms:

  • a matter of    un problème de, une question de
  • as a matter of course    systématiquement
  • as a matter of fact    en fait, à vrai dire
  • dead matter    matière inanimée/inerte
  • for that matter    d'ailleurs
  • foul matter    matières fécales
  • in the matter of    en matière de, pour ce qui concerne
  • matter of course    systématique, naturel ou inévitable (événement)
  • no matter    peu importe!

Deutsch (German)
n. - Angelegenheit, Gegenstand, Materie, Stoff, Inhalt
v. - wichtig sein

idioms:

  • a matter of    nicht mehr als, eine Tatsache
  • as a matter of course    selbstverständlich
  • as a matter of fact    eigentlich
  • dead matter    Ablegesatz
  • for that matter    übrigens
  • foul matter    Ablegesatz
  • in the matter of    was etw. (Akk.) anbelangt
  • matter of course    [etw.] selbstverständlich [tun]
  • no matter    egal ob

Ελληνική (Greek)
n. - ύλη, ουσία, υλικό, ζήτημα, πράγμα, υπόθεση, αιτία, θέμα, λόγος, κείμενο, περιεχόμενο εντύπου, πύο, ακαθαρσία, σημασία
v. - έχω σημασία, υπολογίζομαι, (μτφ.) μετράω, ενδιαφέρω

idioms:

  • a matter of    περίπου, κατά προσέγγιση
  • as a matter of course    αυτονόητος, αναμενόμενος, αυτονόητο ή φυσικό επακόλουθο
  • as a matter of fact    στη πραγματικότητα
  • dead matter    δοκίμια επιστρεφόμενα στον τυπογράφο μετά την εκτύπωση
  • for that matter    όσο γι' αυτό, όσον αφορά αυτό, άλλωστε
  • foul matter    ακαθαρσίες, πύο
  • no matter    δεν πειράζει

Italiano (Italian)
non andare, importare, affare, materia

idioms:

  • a matter of    una questione di
  • as a matter of course    naturalmente
  • as a matter of fact    per dire il vero
  • dead matter    affare chiuso
  • for that matter    per quanto riguarda ciò
  • foul matter    materiale di prima stampa rimandato all'editore
  • no matter    non importa

Português (Portuguese)
n. - matéria (f), negócio (m), importância (f)
v. - significar

idioms:

  • a matter of    uma questão de
  • as a matter of course    fato natural
  • as a matter of fact    na verdade
  • dead matter    assunto encerrado
  • for that matter    no que diz respeito ao assunto
  • foul matter    fato desonesto
  • no matter    não obstante

Русский (Russian)
вещество, материя, сущность, материал, дело, вопрос, повод, иметь значение

idioms:

  • a matter of    приблизительно
  • as a matter of course    само собой разумеющееся
  • as a matter of fact    фактически
  • dead matter    гиблое дело
  • for that matter    что касается этого
  • foul matter    грязное дельце
  • no matter    безразлично

Español (Spanish)
n. - asunto, cuestión, caso, materia, sustancia, material, plomo
v. intr. - pasar, acontecer, importar, ser de importancia

idioms:

  • a matter of    cuestión o cosa de algo
  • as a matter of course    como es natural, como es de rutina, como de costumbre
  • as a matter of fact    en realidad, a decir verdad, de hecho
  • dead matter    asunto muerto, tema finalizado
  • for that matter    en cuanto a eso, en realidad
  • foul matter    asunto muerto, material de impresión redundante
  • in the matter of    en materia de, concerniente a
  • matter of course    como es natural, como es de rutina, como de costumbre, de forma inevitable
  • no matter    no importa

Svenska (Swedish)
n. - materia, ämne, sak, orsak, betydelse, fel (på), sats (typogr.), manuskript, text, var (med.)
v. - betyda, vara (sig) (med.)

中文(简体)(Chinese (Simplified))
事件, 原因, 物质, 有关系, 要紧, 化脓

idioms:

  • a matter of    关于...的事
  • as a matter of course    理所当然的事
  • as a matter of fact    事实上
  • dead matter    结束了不必再提
  • for that matter    就此而言, 而且, 至于那个
  • foul matter    肮脏的事情, 下流的事情
  • no matter    不论...

中文(繁體)(Chinese (Traditional))
n. - 事件, 原因, 物質
v. intr. - 有關係, 要緊, 化膿

idioms:

  • a matter of    關於...的事
  • as a matter of course    理所當然的事
  • as a matter of fact    事實上
  • dead matter    結束了不必再提
  • for that matter    就此而言, 而且, 至於那個
  • foul matter    骯髒的事情, 下流的事情
  • no matter    不論...

한국어 (Korean)
n. - 원료, 본질, 사건, 중점
v. intr. - 중요하다, 상처가 덧나다

idioms:

  • a matter of    문제에 관한, 대략적으로
  • as a matter of course    당연한 일로
  • as a matter of fact    사실상

日本語 (Japanese)
n. - 物質, …質, 問題, 事柄, 困ったこと, 故障, 支障, 事態, 重要性, 内容, 膿, 題材, 原因, 組み版
v. - 重要である, 膿む

idioms:

  • a matter of    問題, およそ…
  • as a matter of course    当然
  • as a matter of fact    実際のところ, 実際は, それどころか
  • for that matter    そのことについては, そういう事なら, そのことならば
  • no matter    たとえ~でも

العربيه (Arabic)
‏(الاسم) مسأله, أهميه, شأن, مادة (فعل) يهم‏

עברית (Hebrew)
n. - ‮חומר, עניין, נושא, מוגלה, דברים מסוג מסוים, תוכן הדברים‬
v. intr. - ‮היה חשוב, הפריש מוגלה‬


 
 

 

Copyrights:

American Heritage Dictionary. The American Heritage® Dictionary of the English Language, Fourth Edition Copyright © 2007, 2000 by Houghton Mifflin Company. Updated in 2009. Published by Houghton Mifflin Company. All rights reserved.  Read more
Britannica Concise Encyclopedia. Britannica Concise Encyclopedia. © 1994-2012 Encyclopædia Britannica, Inc. All rights reserved.  Read more
McGraw-Hill Science & Technology Encyclopedia. McGraw-Hill Encyclopedia of Science and Technology. Copyright © 2005 by The McGraw-Hill Companies, Inc. All rights reserved.  Read more
Roget's Thesaurus. Roget's II: The New Thesaurus, Third Edition by the Editors of the American Heritage® Dictionary Copyright © 1995 byHoughton Mifflin Company. Published by Houghton Mifflin Company. All rights reserved.  Read more
American Heritage Dictionary of Idioms. The American Heritage® Dictionary of Idioms by Christine Ammer. Copyright © 1997 by The Christine Ammer 1992 Trust. Published by Houghton Mifflin Company. All rights reserved.  Read more
Answers Corporation Antonyms by Answers.com. © 1999-present by Answers Corporation. All rights reserved.  Read more
Oxford Dictionary of Philosophy. The Oxford Dictionary of Philosophy. Copyright © 1994, 1996, 2005 by Oxford University Press. All rights reserved.  Read more
Columbia Encyclopedia. The Columbia Electronic Encyclopedia, Sixth Edition Copyright © 2012, Columbia University Press. Licensed from Columbia University Press. All rights reserved. www.cc.columbia.edu/cu/cup/ Read more
Barron's Law Dictionary. Law Dictionary. Copyright © 2003 by Barron's Educational Series, Inc. All rights reserved.  Read more
Oxford Companion to the Mind. The Oxford Companion to the Mind. Second Edition. Copyright © Oxford University Press, 2004. All rights reserved.  Read more
Word Tutor. Copyright © 2004-present by eSpindle Learning, a 501(c) nonprofit organization. All rights reserved.
eSpindle provides personalized spelling and vocabulary tutoring online; sign up free Read more
Dictionary of Cultural Literacy: Science. The New Dictionary of Cultural Literacy, Third Edition Edited by E.D. Hirsch, Jr., Joseph F. Kett, and James Trefil. Copyright © 2002 by Houghton Mifflin Company. Published by Houghton Mifflin. All rights reserved.  Read more
Saunders Veterinary Dictionary. Saunders Comprehensive Veterinary Dictionary 3rd Edition. Copyright © 2007 by D.C. Blood, V.P. Studdert and C.C. Gay, Elsevier. All rights reserved.  Read more
Random House Word Menu. © 2010 Write Brothers Inc. Word Menu is a registered trademark of the Estate of Stephen Glazier. Write Brothers Inc. All rights reserved.  Read more
 Rhymes. Oxford University Press. © 2006, 2007 All rights reserved.  Read more
Bradford's Crossword Solver's Dictionary. Collins Bradford's Crossword Solver's Dictionary © Anne Bradford, 1986, 1993, 1997, 2000, 2003, 2005, 2008 HarperCollins Publishers All rights reserved.  Read more
Wikipedia on Answers.com. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article Matter Read more
Translations. Copyright © 2007, WizCom Technologies Ltd. All rights reserved.  Read more

Follow us
Facebook Twitter
YouTube