2nd Week: Properties of Astrophysical Plasmas B: Difference between revisions
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=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 | Suppose that our system has discrete energies and that <math>n_k</math> is the number of particles occupying the energy level <math>E_k</math>. This two quantities must satisfy | ||
<math>\Omega=-T\sum_{k} \log (\sum_{n_k} | <math>N=\sum_{k}n_k</math> | ||
<math>E_{Total}=\sum_{k}n_k\epsilon_k</math> | |||
. Since we are dealing with fermions, <math>n_k</math> can be 0 or 1. The thermodynamic potential can be written as | |||
<math>\Omega=-T\sum_{k} \log (\sum_{n_k} e^{(\mu-E_k)/kT})</math> |
Revision as of 11:05, 29 January 2009
Occupation probabilities
The 1st law of Thermodynamics in a system (or subsystem) with variable number of particles is
...
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