NFuller
Science Advisor
- 659
- 241
The assumption is that at sufficiently high energies and low densities, the region of phase space excluded by the Pauli exclusion principle is a very small fraction of the total phase space, so we can safely ignore it. Under this assumption the over counting is just a permutation of the particles ##N!##. In the case where this assumption is not valid, we also need to start excluding regions of the phase space. If there are ##G## levels then I believe the over counting will be by a factor of ##N!(G-N)!##.Philip Koeck said:Are you saying that the only correct distributions are Bose-Einstein and Fermi-Dirac (since all particles are either Bosons or Fermions), and Boltzmann can only be an approximation? I think there are many authors who believe that there are "classical" systems that are correctly described even at low temperatures by Boltzmann statistics. You could think of colloids and aerosols, but there's also the gray-zone of gases of atoms, I would say. If you think of He, Ne, Ar etc., shouldn't a classical description become appropriate at some point?
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