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 <math>E_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


<math>N=\sum_{k}n_k</math>
<math>N=\sum_{k}n_k</math>
<math>E_{Total}=\sum_{k}n_k\epsilon_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
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=0}^1 e^{n_k(\mu-\epsilon_k)/kT})</math>


<math>\Omega=-T\sum_{k} \log (\sum_{n_k} e^{(\mu-E_k)/kT})</math>
<math>\Omega=-T\sum_{k} \log (1 + e^{(\mu-\epsilon_k)/kT})</math>

Revision as of 11:09, 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