2nd Week: Properties of Astrophysical Plasmas B: Difference between revisions

From PhyWiki
Jump to navigation Jump to search
No edit summary
No edit summary
Line 7: Line 7:


=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>. Since we are dealing with fermions, <math>n_k</math> can be 0 or 1. The thermodynamic potential can be written as
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}\exp{\mu-E_k})</math>
<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