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 Übersetzung für 'degenerate matter' von Englisch nach Deutsch
NOUN   degenerate matter [phys.] | -
degenerate matterverdorbenes Material {n}
phys.
degenerate matter
entartete Materie {f}
astron.
degenerate matter
degenerierte Materie {f}
Teiltreffer
degeneratedegenerierter Mensch {m}
to degenerateverflachen
degeneratedekadenter Mensch {m}
to degenerateentarten
68
to degenerateentkoppeln
9
to degenerateverkommen
144
to degenerategegenkoppeln
math.
degenerate {adj}
ausgeartet
169
biol.med.
to degenerate
8
abarten [fachspr.] [sonst selten] [von der Art abweichen]
to degeneratezerfallen
19
to degeneratesichAkk. zersetzen
to degenerateverderben
14
degenerate {adj}entartet
215
to degeneratesittlich herunterkommen
to degenerateausarten
196
to degenerateherabsinken
6
to degenerateverfallen
66
to degeneratenachlassen
12
degenerate {adj}heruntergekommen
319
degenerate {adj}degeneriert
119
23 Übersetzungen
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Anwendungsbeispiele Englisch
  • ... 19 October 1910 – 21 August 1995) At the University of Cambridge, he developed a theoretical model explaining the structure of white dwarf stars that took into account the relativistic variation of mass with the velocities of electrons that comprise their degenerate matter.
  • A degenerate mass whose fermions have velocities close to the speed of light (particle kinetic energy larger than its rest mass energy) is called relativistic degenerate matter.
  • If a white dwarf, which is composed almost entirely of degenerate matter, can gain mass from a companion, the increasing temperature and density of material in its core will ignite carbon fusion if the star's mass approaches the Chandrasekhar limit.
  • A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter.
  • 3 times the mass of the Sun the helium core becomes a region of degenerate matter that does not contribute to the generation of energy.

  • If the mass of the collapsing part of the star is below the Tolman–Oppenheimer–Volkoff (TOV) limit for neutron-degenerate matter, the end product is a compact star – either a white dwarf (for masses below the Chandrasekhar limit) or a neutron star or a (hypothetical) quark star.
  • As the hydrogen in the core is exhausted, some of the helium left behind is instead compacted into degenerate matter, supported against gravitational collapse by quantum mechanical pressure rather than thermal pressure.
  • One model describes the core as superfluid neutron-degenerate matter (mostly neutrons, with some protons and electrons).
  • Planets and stars have radial density gradients from their lower density surfaces to their much denser compressed cores. Degenerate matter objects (white dwarfs; neutron star pulsars) have radial density gradients plus relativistic corrections.
  • The binary could help our understanding of neutron degenerate matter; the current median mass, if confirmed, would exclude any "soft" equation of state for such matter.

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