Particle

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Arc welders need to protect themselves from welding sparks, which are heated metal particles that fly off the welding surface.

In the physical sciences, a particle is a small localized object to which can be ascribed several physical or chemical properties such as volume or mass.[2] The word is rather general in meaning, and is refined as needed by various scientific fields. Something that is composed of particles may be referred to as particulate,[3] although this term is generally used to refer to a suspension of unconnected particles, rather than a connected particle aggregation.

Whether objects can be considered particles depends on the scale of the context; if an object's own size is small or negligible, or if geometrical properties and structure are irrelevant, then it can often be considered a particle.[4] For example, grains of sand on a beach can be considered particles because the size of one grain of sand (~1 mm) is negligible compared to the beach, and the features of individual grains of sand are usually irrelevant to the problem at hand. However, grains of sand would not be considered particles if compared to buckyballs (~1 nm).

Conceptual properties

Particles are very often represented as dots. This figure could represent the movement of atoms in a gas, people in crowds or stars in the night sky.

The concept of particles is particularly useful when modelling nature, as the full treatment of many phenomena is complex.[5] It can be used to make simplifying assumptions concerning the processes involved. Francis Sears and Mark Zemansky, in University Physics, give the example of calculating the landing location and velocity of a baseball thrown in the air. They gradually strip the baseball of most of its properties, by first idealizing it as a rigid smooth sphere, then by neglecting rotation, buoyancy and friction, ultimately reducing the problem to the ballistics of a classical point particle.[6]

Treatment of large numbers of particles is the realm of statistical physics.[7] When studied in the context of an extremely small scale, quantum mechanics becomes important and gives rise to several phenomena demonstrated in the particle in a box model[8][9] including wave–particle duality,[10][11] or theoretical considerations, such a whether particles can be considered distinct or identical.[12][13]

Size

Galaxies are so large that stars can be considered particles relative to them

The term "particle" is usually applied differently to three classes of sizes. The term macroscopic particle, usually refers to particles much larger than atoms and molecules. These are usually abstracted as point-like particles, even though they have volumes, shapes, structures, etc. Examples of macroscopic particles would include dust, sand, pieces of debris during a car accident, or even objects as big as the stars of a galaxy.[14][15] Another type, microscopic particles usually refers to particles of sizes ranging from atoms to molecules, such as carbon dioxide, nanoparticles, and colloidal particles. The smallest of particles are the subatomic particles, which refer to particles smaller than atoms.[16] These would include particles such as the constituents of atoms – protons, neutrons, and electrons – as well as other types of particles which can only be produced in particle accelerators or cosmic rays.

Composition

A proton is composed of three quarks.

Particles can also be classified according to composition. Composite particles refer to particles that have composition – that is particles which are made of other particles.[17] For example, a carbon-14 atom is made of six protons, eight neutrons, and six electrons. By contrast, elementary particles (also called fundamental particles) refer to particles that are not made of other particles.[18] According to our current understanding of the world, only a very small number of these exist, such as the leptons, quarks or gluons. However it is possible that some of these might turn up to be composite particles after all, and merely appear to be elementary for the moment.[19] While composite particles can very often be considered point-like, elementary particles are truly punctual.[20]

Stability

Both elementary (such as muons) and composite particles (such as Sigma baryons), are known to undergo particle decay. Those that don't are called stable particles, such as the electron or a helium-4 nucleus. The lifetime of stable particles can be either infinite or large enough to hinder attempts to observe such decays. In the later case, those particles are called "observationally stable". In general, a particle decays from a high-energy state to a lower-energy state by emitting some form of radiation, such as the emission of photons.

N-body simulation

The Millennium Run is a N = ~109 simulation of the universe, from the Big Bang until the present state. Each "particle" represents approximately a billion solar masses of dark matter.[1]

In computational physics, N-body simulations (also called N-particle simulations) are simulations of dynamical systems of particles under the influence of certain conditions, such as being subject to gravity.[21] These simulations are very common in cosmology and computational fluid dynamics.

N refers to the number of particles considered. As simulations with higher N are more computationally intensive, systems with large numbers of actual particles will often be approximated to a smaller number of particles, and simulation algorithms need to be optimized through various methods.[21]

Distribution of particles

Colloidal particles are the components of a colloid. A colloid is a substance microscopically dispersed evenly throughout another substance.[22] Such colloidal system can be solid, liquid, or gaseous; as well as continuous or dispersed. The dispersed-phase particles have a diameter of between approximately 5 and 200 nanometers.[23] Soluble particles smaller than this will form a solution as opposed to a colloid. Colloidal systems (also called colloidal solutions or colloidal suspensions) are the subject of interface and colloid science. Suspended solids may be held in a liquid, while solid or liquid particles suspended in a gas together form an aerosol. Particles may also be suspended in the form of atmospheric particulate matter, which may constitute air pollution. Larger particles can similarly form marine debris or space debris. A conglomeration of discrete solid, macroscopic particles may be described as a granular material.

See also

References

  1. V. Springel et al. (2005). "Simulating the joint evolution of quasars, galaxies and their large-scale distribution". Nature 435 (7042): 629–636. arXiv:astro-ph/0504097. Bibcode:2005Natur.435..629S. doi:10.1038/nature03597. PMID 15931216. 
  2. "Particle". AMS Glossary. American Meteorological Society. 
  3. See T. William Lambe, Robert V. Whitman, Soil Mechanics (1969), p. 18, stating: "The word 'particulate' means 'of or pertaining to a system of particles'" .
  4. "Particle". Dictionary.com. Retrieved 2010-02-08. 
  5. F. W. Sears, M. W. Zemanski (1964). "Equilibrium of a Particle". University Physics (3rd ed.). Addison-Wesley. pp. 26–27. LCCN 6315265. 
  6. F. W. Sears, M. W. Zemanski (1964). "Equilibrium of a Particle". University Physics (3rd ed.). Addison-Wesley. p. 27. LCCN 6315265. "A body whose rotation is ignored as irrelevant is called a particle. A particle may be so small that it is an approximation to a point, or it may be of any size, provided that the action lines of all the forces acting on it intersect in one point." 
  7. F. Reif (1965). "Statistical Description of Systems of Particles". Fundamentals of Statistical and Thermal Dynamics. McGraw-Hill. pp. 47ff. 
  8. R. Eisberg, R. Resnick (1985). "Solutions of Time-Independent Schroedinger Equations". Quantum Physics of Atoms, Molecules, Solids, Nuclei, and Particles (2nd ed.). John Wiley & Sons. pp. 214–226. ISBN 0-471-87373-X. 
  9. F. Reif (1965). "Quantum Statistics of Ideal Gases – Quantum States of a Single Particle". Fundamentals of Statistical and Thermal Dynamics. McGraw-Hill. pp. vii–x. 
  10. R. Eisberg, R. Resnick (1985). "Photons—Particlelike Properties of Radiation". Quantum Physics of Atoms, Molecules, Solids, Nuclei, and Particles. (2nd ed.). John Wiley & Sons. pp. 26–54. ISBN 0-471-87373-X. 
  11. R. Eisberg, R. Resnick (1985). "de Broglie's Postulate—Wavelike Properties of Particles". Quantum Physics of Atoms, Molecules, Solids, Nuclei, and Particles (2nd ed.). John Wiley & Sons. pp. 55–84. ISBN 0-471-87373-X. 
  12. F. Reif (1965). "Quantum Statistics of Ideal Gases – Identical Particles and Symmetry Requirements". Fundamentals of Statistical and Thermal Dynamics. McGraw-Hill. pp. 331ff. 
  13. F. Reif (1965). "Quantum Statistics of Ideal Gases – Physical Implications of the Quantum-Mechanical Enumeration of States". Fundamentals of Statistical and Thermal Dynamics. McGraw-Hill. pp. 353–360. 
  14. J. Dubinksi (2003). "Galaxy Dynamics and Cosmology on Mckenzie". Canadian Institute for Theoretical Astrophysics. Retrieved 2011-02-24. 
  15. G. Coppola, F. La Barbera, M. Capaccioli (2009). "Sérsic galaxy with Sérsic halo models of early-type galaxies: A tool for N-body simulations". Publications of the Astronomical Society of the Pacific 121 (879): 437. arXiv:0903.4758. Bibcode:2009PASP..121..437C. doi:10.1086/599288. 
  16. "Subatomic particle". YourDictionary.com. Retrieved 2010-02-08. 
  17. "Composite particle". YourDictionary.com. Retrieved 2010-02-08. 
  18. "Elementary particle". YourDictionary.com. Retrieved 2010-02-08. 
  19. I. A. D'Souza, C. S. Kalman (1992). Preons: Models of Leptons, Quarks and Gauge Bosons as Composite Objects. World Scientific. ISBN 981-02-1019-1. 
  20. US National Research Council (1990). "What is an elementary particle?". Elementary-Particle Physics. US National Research Council. p. 19. ISBN 0-309-03576-7. 
  21. 21.0 21.1 A. Graps (20 March 2000). "N-Body / Particle Simulation Methods". Retrieved 2011-02-24. 
  22. "Colloid". Encyclopædia Britannica. Retrieved 2011-02-24. 
  23. I. N. Levine (2001). Physical Chemistry (5th ed.). McGraw-Hill. p. 955. ISBN 0-07-231808-2. 

Further reading

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