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Degenerate matter - Wikipedia, the free encyclopedia
Degenerate matter is matter which has such extraordinarily high density that the dominant contribution to its pressure rises from the Pauli exclusion principle. The pressure maintained by a body of d...
en.wikipedia.org/wiki/Degenerate_matter |
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Degenerate gas - Topic:Astronomy - Online Encyclopedia ... DEGENERATE GAS; A degenerate gas is one that is super-compressed and very dense. The molecules of this degenerate gas are virtually touching one another and the gas acts much like a solid.
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When gas become super-compressed, particles bump right up against each other to produce a kind of gas, called a degenerate gas, that behaves more like a solid. Normal gas exerts higher pressure when it is heated and expands, but the pressure in a degenerate gas does not depend on the temperature.
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degenerate gas super-compressed gas that behaves more like a solid and whose properties must be described by quantum mechanics. The pressure of degenerate gas does not depend on the temperature.
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[Archive] What is a degenerate gas? Astrophysics ... hi, I'm studying stellar structures and there's always mention of a degenerate gas (I think it goes by other names such as degenerate electron gas or cold gas). The only time I've heard the word degenerate is in the context of quantum mechanics, but I think this...
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Supernova Ejection (Continued) ... The energy deposited in the lower layers of the envelope creates a superstrong shock wave that runs outward through the envelope toward the star's surface. ... As the shock wave runs outward, it heats the envelope, induces explosive nuclear burning, and ejects the envelope at speeds of...
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a cloud of gas around a planet. ... an expanding shell of gas about a star. ... The rapid fusion of helium in the electron-degenerate helium core of a red giant...
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SAO/NASA ADS Astronomy Abstract Service ... Title:; The minimum pressure of a degenerate electron gas ... Publication:; Monthly Notices of the Royal Astronomical Society, Vol. 92, p.651 (MNRAS Homepage)
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A closed form for the static dielectric function of a relativistic degenerate electron gas is given on the basis of Chin's (1977) divergence-free formalism. An expression is derived for the electronic stopping power.
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We report on the observation of a highly degenerate, strongly interacting Fermi gas of atoms. Fermionic 6Li atoms in an optical trap are evaporatively cooled to degeneracy using a magnetic field to induce strong, resonant interactions.
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