Thermal Physics |
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Page 223
... Fermi energy : TEF . The orbitals of energy lower than the Fermi energy will be almost entirely occupied when this inequality is satisfied , and the orbitals of higher energy will be almost entirely vacant . An orbital is occupied fully ...
... Fermi energy : TEF . The orbitals of energy lower than the Fermi energy will be almost entirely occupied when this inequality is satisfied , and the orbitals of higher energy will be almost entirely vacant . An orbital is occupied fully ...
Page 242
... energy is much lower than the Fermi energy . Are the electron energies in the relativistic regime ? We are concerned with this question because our development of the theory of the Fermi gas has used the nonrelativistic expression p2 ...
... energy is much lower than the Fermi energy . Are the electron energies in the relativistic regime ? We are concerned with this question because our development of the theory of the Fermi gas has used the nonrelativistic expression p2 ...
Page 415
... Fermi energy , 142 , 236 Fermi energy parameters ( table ) , 236 Fermi gas , application to white dwarfs , 240 chemical potential , 232 , 235 , 382 degenerate , 223 energy , 230 equation of state , 317 ground state , 225 He3 , 239 heat ...
... Fermi energy , 142 , 236 Fermi energy parameters ( table ) , 236 Fermi gas , application to white dwarfs , 240 chemical potential , 232 , 235 , 382 degenerate , 223 energy , 230 equation of state , 317 ground state , 225 He3 , 239 heat ...
Contents
STATES OF THE MODEL SYSTEM | 11 |
AN ELEMENTARY SOLUBLE SYSTEM | 17 |
SHARP PEAK OF gN | 19 |
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approximation Boltzmann bosons calculated Carnot cycle chemical potential classical regime closed system cm³ combined system concentration defined definition denote derivative diffusive contact dipole distribution function electric field electron energy levels ensemble entropy equal equation equilibrium ergs example expansion experimental Fermi energy Fermi gas Fermi-Dirac fermions Figure fluctuations flux fractional free energy free particle frequency gases given grand sum He¹ He³ heat capacity helium ideal gas law increase integral isothermal kinetic lattice liquid low temperature m₁ magnetic field magnetic moment model system molecule N₁ negative temperature number of accessible number of atoms number of particles occupied P₁ partition function photons plotted pressure probable configuration Problem properties quantity quantum number reservoir result spin excess superfluid system in thermal term thermal average thermal contact thermodynamic potential total number U₁ unit velocity versus volume white dwarf ат