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1 faktor kemerosotan
degeneracy factor -
2 степень вырождения
Русско-английский словарь по микроэлектронике > степень вырождения
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3 степень вырождения
degeneracy factor, degree of degeneracyРусско-английский словарь по радиоэлектронике > степень вырождения
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4 степень вырождения
1) Engineering: degeneracy, degeneration factor, degree of degeneracy2) Mathematics: nullity3) Metallurgy: degeneracy multiplicity4) Electronics: degeneracy factorУниверсальный русско-английский словарь > степень вырождения
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5 степень вырождения
degree of degeneracy, degeneracy factorРусско-английский словарь по электронике > степень вырождения
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6 Entartungsfaktor
Entartungsfaktor m degeneracy factorDeutsch-Englisch Wörterbuch der Elektrotechnik und Elektronik > Entartungsfaktor
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7 Spinentartungsfaktor
Spinentartungsfaktor m spin degeneracy factorDeutsch-Englisch Wörterbuch der Elektrotechnik und Elektronik > Spinentartungsfaktor
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8 степень вырождения
degeneracy, degree of degeneracy, degeneration factorРусско-английский политехнический словарь > степень вырождения
См. также в других словарях:
Degeneracy (graph theory) — In graph theory, a k degenerate graph is an undirected graph in which every subgraph has a vertex of degree at most k: that is, some vertex in the subgraph touches k or fewer of the subgraph s edges. The degeneracy of a graph is the smallest… … Wikipedia
Electron degeneracy pressure — is a consequence of the Pauli exclusion principle, which states that two fermions cannot occupy the same quantum state at the same time. The force provided by this pressure sets a limit on how much matter can be squeezed together without it… … Wikipedia
Landé g-factor — In physics, the Landé g factor is a particular example of a g factor, namely for an electron with both spin and orbital angular momenta. It is named after Alfred Landé, who first described it in 1921.In atomic physics, it is a multiplicative term … Wikipedia
Partition function (statistical mechanics) — For other uses, see Partition function (disambiguation). Partition function describe the statistical properties of a system in thermodynamic equilibrium. It is a function of temperature and other parameters, such as the volume enclosing a gas.… … Wikipedia
Maxwell–Boltzmann distribution — Maxwell–Boltzmann Probability density function Cumulative distribution function parameters … Wikipedia
Density of states — Condensed matter physics Phases · Phase tr … Wikipedia
cosmos — /koz meuhs, mohs/, n., pl. cosmos, cosmoses for 2, 4. 1. the world or universe regarded as an orderly, harmonious system. 2. a complete, orderly, harmonious system. 3. order; harmony. 4. any composite plant of the genus Cosmos, of tropical… … Universalium
Perturbation theory (quantum mechanics) — In quantum mechanics, perturbation theory is a set of approximation schemes directly related to mathematical perturbation for describing a complicated quantum system in terms of a simpler one. The idea is to start with a simple system for which a … Wikipedia
Chandrasekhar limit — When a star starts running out of fuel, it usually cools off and collapses (possibly with a supernova) into one of three compact forms, depending on its total mass: a White Dwarf, a big lump of Carbon and Oxygen atoms, almost like one huge… … Wikipedia
White dwarf — For other uses, see White dwarf (disambiguation). Image of Sirius A and Sirius B taken by the Hubble Space Telescope. Sirius B, which is a white dwarf, can be seen as a faint pinprick of light to the lower left of the much brighter Sirius A … Wikipedia
Type II supernova — The expanding remnant of SN 1987A, a Type II P supernova in the Large Magellanic Cloud. NASA image. A Type II supernova (plural: supernovae) results from the rapid collapse and violent explosion of a massive star. A star must have at least 9… … Wikipedia