An Etymological Dictionary of Astronomy and Astrophysics

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory



<< < bif gro sys > >>

Number of Results: 47 Search : theory
bifurcation theory
  نگره‌ی ِ دوگلش   
negare-ye dogaleš

Fr.: théorie de bifurcation   

1) A theory which studies how, in certain nonlinear systems, there may be paths and shifts in behavior dependent on small changes in circumstances or the current position of the system.
2) Math.: The study of the behavior of a solution of a nonlinear problem in the neighborhood of a known solution, particularly as a parameter varies.

bifurcation; → theory.

Big Bang theory
  نگره‌ی ِ مه بانگ، ~ بیگ بنگ   
negare-ye Meh Bâng, ~ Big Bang

Fr.: théorie du big bang   

Big Bang; → theory.

Cartesian vortex theory
  نگره‌ی ِ گردشار ِ دکارت   
negare-ye gerdšâr-e Descartes

Fr.: théorie des vortex de Descartes   

A mechanical model put forward before Newton's theory of gravity to explain the revolution of the planets around the Sun. Descartes in his 1644 Principia Philosophiae postulated that the space between the Sun and the planets is filled with matter in the form of a fluid. The fluid rotates in countless whirlpools, one for each planet, thus carrying the planets along in their flow. The vortices vary in size and are contiguous as well as nested. Descartes believed that two objects can exert force on each other only when they are in physical contact. This is why he postulated that space is filled with matter. Newton refuted the vortex theory, using the principle of → action at a distance on which relies his → law of universal gravitation.

Cartesian; → vortex; → theory.

category theory
  نگره‌ی ِ کتاگر   
negare-ye katâgor

Fr.: théorie des catégories   

A theory that deals with the concept of → category and generalizes the → set theory.

category; → theory.

chaos theory
  نگره‌ی ِ ورشون   
negare-ye varšun

Fr.: théorie du chaos   

The theory of unpredictable behavior that can arise in systems obeying deterministic scientific laws.

theory; → chaos.

classical field theory
  نگره‌ی ِ کلاسیک ِ میدان   
negare-ye klâsik-e meydân

Fr.: théorie classique des champs   

The theory that studies distributions of → energy, → matter, and other physical quantities under circumstances where their discrete nature is unimportant. Classical field theory traditionally includes → Newtonian mechanics, Maxwell's → electromagnetic theory, and Einstein's theory of → general relativity. The main scope of classical field theory is to construct the mathematical description of → dynamical systems with an infinite number of degrees of freedom. The word "classical" is used in contrast to those field theories that incorporate → quantum mechanics (→ quantum field theory). Classical field theories are usually categorized as → non-relativistic and → relativistic.

classical; → field; → theory.

corpuscular theory of light
  نگره‌ی ِ کرپولی ِ نور   
negare-ye karpuli-ye nur

Fr.: théorie corpusculaire de la lumière   

Newton's theory according to which light is made up of point-like particles without any mass. It failed to explains several phenomena: simultaneous reflection and refraction at a semi-transparent boundary, interference, diffraction and polarization. Moreover, it requested that the speed of light be greater in a denser medium than in a rarer medium; this prediction is contrary to experimental results. In 1924 Louis de Broglie postulated that matter has not only a corpuscular nature but also a wave nature, and subsequent experiments confirmed de Broglie's model.

Corpuscular, adj. from → corpuscle; → theory, → light.

density wave theory
  نگره‌ی ِ موج ِ چگالی   
negare-ye mowj-e cagâli

Fr.: théorie des ondes de densité   

One possible explanation for → spiral arms, first put forward by B. Lindblad in about 1925 and developed later by C.C. Lin and F. H. Shu. According to this theory, spiral arms are not material structures, but regions of somewhat enhanced density, created by → density waves. Density waves are perturbations amplified by the self-gravity of the → galactic disk. The perturbation results from natural non-asymmetry in the disk and enhanced by environmental processes, such as galaxy encounters. Density waves rotate around the → galactic center and periodically compress the disk material upon their passage. If the spiral arms were rigid structures rotating like a pinwheel, the → differential rotation of the galaxy would wind up the arms completely in a relatively short time (with respect to the age of the galaxy), → winding problem. Inside the region defined by the → corotation radius, density waves rotate more slowly than the galaxy's stars and gas; outside that region they rotate faster.
As the density waves rotate, they are overtaken by the individual stars and nebulae/molecular clouds that are rotating around the galaxy at a higher rate. The molecular clouds passing through the density wave are subjected to compression because it is a region of higher density. This triggers the formation of clusters of new stars, which continue to move through the density wave.
The short-lived stars die, most likely as supernovae, before they can leave the spiral density wave. But the longer-lived stars that are formed pass through the density wave and eventually emerge on its front side and continue on their way as a slowly dissipating cluster of stars. Density wave theory explains much of the spiral structure that we see, but there are some problems. First, computer simulations with density waves tend to produce very orderly "grand design" spirals with a well-defined, wrapped 2-arm structure. But there are many spiral galaxies that have a more complex structure than this (→ flocculent spiral galaxy). Second, density wave theory assumes the existence of spiral density waves and then explores the consequences.
See also: → stochastic self-propagating star formation.

density; → wave; → theory.

deterministic theory
  نگره‌ی ِ آترم‌باور   
negare-ye âtarmbâvar

Fr.: théorie déterministe   

A theory in which specification of the initial value of all relevant variables of the system is sufficient to calculate the past values and to predict the future values of such variables for any arbitrary time. Moreover, it is possible, for any arbitrary time, to assign a value to all the variables characterizing the system. In quantum mechanics, the time evolution of the → wave function, governed by the → Schrodinger equation, is deterministic. Quantum mechanics, however, is a non deterministic theory because of the probabilistic nature of the predictions for the values of the → observables of a quantum system.

deterministic; → theory.

Dvali-Gabadadze-Porrati theory (DGP)
  نگره‌ی ِ دوالی-گبزده-پراتی   
negare-ye Dvali-Gabadadze-Porrati

Fr.: théorie de Dvali-Gabadadze-Porrati   

A → braneworld theory in which the → space-time is locally embedded in a five dimensional space, the → bulk, and has as a key aspect leakage of gravitational energy into the bulk. More specifically, the → graviton is pinned to a four-dimensional braneworld by intrinsic curvature terms induced by quantum matter fluctuations. But as it propagates over large distances, the graviton eventually evaporates off the brane into an infinite volume, five-dimensional Minkowski bulk. Therefore, the DGP braneworld theory is a model in a class of theories in which gravity deviates from conventional → General Relativity not at short distances, but rather at long distances. This means that at those distances General Relativity cannot correctly describe gravitational interactions. This model has various cosmologically interesting features. Particularly in the model with five dimensional bulk, the → accelerating expansion of the Universe at late epoch is realized without introducing the → cosmological constant (see, e.g., A. Lue, 2002, arxiv.0208169, T. Tanaka, 2003, arXiv.0305031).

G. Dvali, G. Gabadadze and M. Porrati, 2000, Phys. Lett. 485B, 208.

dynamo theory
  نگره‌ی ِ توانزا   
negare-ye tavânzâ

Fr.: théorie de la dynamo   

Branch of magnetohydrodynamics concerned with self-excitation of magnetic fields in any large rotating mass of conducting fluid in motion (usually turbulent). Self-exciting dynamo action is believed to account for magnetic fields at the planetary, stellar, and galactic scales.

dynamo; → theory.

Einstein's theory of specific heat
  نگره‌ی ِ گرمای ِ آبیزه‌ی ِ اینشتین   
negare-ye garmâ-ye âbize-ye Einstein

Fr.: théorie de la chaleur spécifique d'Einstein   

Same as → Einstein model.

Einstein; → theory; → specific heat.

electromagnetic theory
  نگره‌ی ِ برقامغناتی   
negare-ye barqâmeqnâti

Fr.: théorie électromagnétique   

The description of combined electric and magnetic fields mainly by → Maxwell's equations. Same as → electromagnetism.

electromagnetic; → theory.

electromagnetic theory of light
  نگره‌ی ِ برقامغناتی ِ نور   
negare-ye barqâmeqnâti-ye nur

Fr.: théorie électromagnétique de la lumière   

The theory describing light as a wave phenomenon resulting from the combination of two electric and magnetic fields vibrating transversely and mutually at right angles. → electromagnetic radiation; → electromagnetic wave; → Maxwell's equations.

electromagnetic; → theory; → light.

epicyclic theory
  نگره‌ی ِ اپی-چرخه‌ای   
negare-ye apicarxe-yi

Fr.: théorie épicyclique   

The theory that describes the Galactic dynamics, that is the orbits of stars and gas clouds in the → Galactic disk, as well as the spiral → density wave. Formulated by Bertil Lindblad (1895-1965), the epicyclic theory assumes that orbits are circular with small deviations. Star orbits are described by the superposition of two motions: i) a rotation of the star (epicenter) around the Galactic center at the circular angular velocity, Ω, and ii) a retrograde elliptical motion at → epicyclic frequency, κ. The epicyclic motion in the Galactic plane occurs in a retrograde sense to conserve → angular momentum. In general Ω and κ are different and, therefore, orbits do not close. However, seen by an observer who rotates with the epicenter, orbits are closed ellipses.

epicyclic; → theory.

field theory
  نگره‌ی ِ میدان   
negare-ye meydân

Fr.: théorie des champs   

1) A theory which uses the concept of → field to describe physical phenomena. It consists of two types: → classical field theory and → quantum field theory.
2) Math.: A branch of mathematics which studies the → fields.

field; → theory.

gauge theory
  نگره‌ی ِ گز   
negare-ye gaz (#)

Fr.: théorie de jauge   

A field theory in which it is possible to perform a transformation without altering any measurable physical quantity.

gauge; → theory.

grand unified theory (GUT)
  نگره‌ی ِ یگانش ِ بزرگ   
negare-ye yegâneš-e bozorg (#)

Fr.: théorie de la grande unification   

Any physical theory that unites the strong, electromagnetic, and weak interactions at high energy. It is hoped that GUTs can ultimately be extended to incorporate gravity. → theory of everything.

M.E. graunt, from O.Fr. grant, grand, from L. grandis "big, great," also "full-grown;" unified, p.p. of → unify; → theory.

Negâré, → theory; yegâneš, verbal noun of yegânestan, → unify; bozorggreat.

graph theory
  نگره‌ی ِ نگاره   
negare-ye negâré

Fr.: théorie des graphes   

The branch of → mathematics dealing with → graphs. In particular, it involves the ways in which sets of points (→ vertex) can be connected by lines or arcs (→ edge).

graph; → theory.

gravitational-field theory
  نگره‌ی ِ میدان ِ گرانشی   
negare-ye meydân-e gerâneši (#)

Fr.: théorie de champ gravitationnel   

A theory that treats gravity as a field rather than a force acting at a distance.

gravitational; → field.

<< < bif gro sys > >>