Fermi gas

E57419

A Fermi gas is a quantum many-particle system composed of fermions that obey Fermi–Dirac statistics, often used to model electrons in metals, neutrons in neutron stars, and ultracold atomic gases.

Aliases (1)

Statements (49)
Predicate Object
instanceOf ideal quantum gas
quantum many-body system
theoretical physics model
applicableTo electrons in a metal conduction band
neutron matter in neutron stars (approximation)
nucleons in atomic nuclei (approximation)
trapped ultracold fermionic atoms
assumes indistinguishable fermions
occupation numbers 0 or 1 per state
characterizedBy Fermi energy
Fermi momentum
Fermi temperature
composedOf fermions
contrastedWith Bose–Einstein gas
describedIn statistical mechanics
equationOfStateDependsOn particle density
spin degeneracy
temperature
hasDistributionFunction Fermi–Dirac distribution
hasProperty at most one fermion per single-particle quantum state
particles obey Pauli exclusion principle
pressure persists at zero temperature
quantum degeneracy at low temperature
supports Fermi pressure
hasVariant degenerate Fermi gas
ideal Fermi gas
interacting Fermi gas
non-interacting Fermi gas
relativistic Fermi gas
spin-polarized Fermi gas
limitCase classical ideal gas at high temperature and low density
namedAfter Enrico Fermi
obeys Fermi–Dirac statistics
relatedToConcept Bose gas
Fermi liquid
Fermi surface
Pauli exclusion principle
degeneracy pressure
quantum degeneracy
temperatureRegime quantum effects dominate below Fermi temperature
usedIn astrophysics
cold atom physics
condensed matter physics
nuclear physics
usedToExplain electronic heat capacity of metals
stability of white dwarfs and neutron stars via degeneracy pressure
usedToModel electrons in metals
neutrons in neutron stars
ultracold atomic gases

Referenced by (2)
Subject (surface form when different) Predicate
Pauli exclusion principle ("Fermi gas model")
isBasisFor
Bose–Einstein condensate
isRelatedTo

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