Evaluating the average occupancy of each energy state is much simpler than in the Maxwell-Boltzmann example since each macrostate has a weight of 1. The average occupancy is just the sum of the numbers of particles in a given energy state over all the 5 distributions divided by 5.
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Index Reference Blatt Ch. 11 | ||||
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The average distribution of 9 units of energy among 6 identical particles
For fermions, there are only 5 possible distributions of 9 units of energy among 6 particles compared to 26 possible distributions for classical particles. To get a distribution function of the number of particles as a function of energy, the average population of each energy state must be taken. The average for each of the 9 states is shown above compared to the results obtained by Maxwell-Boltzmann statistics and Bose-Einstein statistics . Low energy states are less probable with Fermi-Dirac statistics than with the Maxwell-Boltzmann statistics while mid-range energies are more probable. While that difference is not dramatic in this example for a small number of particles, it becomes very dramatic with large numbers and low temperatures. At absolute zero all of the possible energy states up to a level called the Fermi energy are occupied, and all the levels above the Fermi energy are vacant. |
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