Terms: Electron Pressure (2090), fermi pressure (220), fermi energy (46300), fermi temperature (775), fermi gas (26000), fermi momentum (1350),
Terms: fermi gases (14100), fermi edge (1180), fermi surface (66200), fermi surfaces (10000), degeneracy pressure (3020), fermi wavelength (668), quantum gases (15700), relativistic fermi (258),
Terms: compressibility (196000), internal pressure (197000), lattice pressure (28), lattice energy (14900), pauli pressure (28), quantum pressure (370),
Terms: million atmospheres (659), gigapascal (615), megapascal (1490), terapascal (103),
1 gigapascal = 9,869.2316931 atmosphere [standard]
1 terapascal = 9,869,231.6931427 atmosphere [standard]
Terms: compressive strength (275000), tensile strength (1340000), quartzlike carbon dioxide (13),
Boolean: "fermi energy" AND (sodium OR potassium) (782), "fermi energy" AND pressure (2120), "fermi energy" AND megabars (15), "fermi energy" AND compressibility (173),
Terms: solid state physics (741000), condensed matter physics (378000), electron density (339000),
Terms: closely packed electrons (12), white dwarfs (123000), electrons in metals (2620),
[cond-mat/0303047] Electron and nuclear pressures in liquid metals and plasmas
Terms: zero-temperature pressure (16), electron gas (85800),
Free electron gas under high pressure
Mechanical stability of a strongly interacting Fermi gas of atoms
Statistical Physics - Diamagnetism in free electron metals
for4He nuclei at a density of 100 g/cm3 and ne = 8x1024 cm-3
Cosmology Class at Berkeley - Phys112
Freiburg - Statistics and Thermodynamics, Stochastic Processes -
Matter, Energy, and Radiation Hydrodynamics
The total pressure present is the sum of the Fermi pressure, the kinetic pressure of the Boltzmann gas consisting of the nuclei and non-degenerate electrons, and the pressure of the photon Bose gas. Similarly, the energy density is the sum of the contributions from the Fermi, Boltzmann, and Bose gases that are present.
Terms: detonation wave (4120), detonation waves (2500), standing waves (149000), shock waves (580000), standing wave (151000), shock wave (744000),
Henri Jansen Notes
the Fermi energy is the amount of energy needed to subtract or add an electron to the system at zero temperature. These quantities are called the ionization energy and electron affinity. They are the same in a metal, but different in an insulator. Therefore, in an insulator the only correct definition of the Fermi energy is the zero temperature limit of the chemical potential
Terms: ionization energy (53900), electron affinity (41700),