2nd Week: Properties of Astrophysical Plasmas B: Difference between revisions
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===Maxwell-Boltzmann=== | |||
=Fermi-Dirac= | |||
===Fermi-Dirac=== | |||
Suppose that our system has discrete energies and that <math>n_k</math> is the number of particles occupying the energy level <math>\epsilon_k</math>. This two quantities must satisfy | Suppose that our system has discrete energies and that <math>n_k</math> is the number of particles occupying the energy level <math>\epsilon_k</math>. This two quantities must satisfy | ||
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<math>\Omega=-T\sum_{k} \log (1 + e^{(\mu-\epsilon_k)/kT})</math> | <math>\Omega=-T\sum_{k} \log (1 + e^{(\mu-\epsilon_k)/kT})</math> | ||
===Bose-Einstein=== |
Revision as of 11:12, 29 January 2009
Occupation probabilities
The 1st law of Thermodynamics in a system (or subsystem) with variable number of particles is
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Maxwell-Boltzmann
Fermi-Dirac
Suppose that our system has discrete energies and that is the number of particles occupying the energy level . This two quantities must satisfy
Since we are dealing with fermions, can be 0 or 1. The thermodynamic potential can be written as