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

Bose-Einstein