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Elementary Properties of a Degenerate Fermi Gas

  • V. Kourganoff
Part of the Geophysics and Astrophysics Monographs book series (GAAM, volume 17)

Abstract

We deal in this section with relatively elementary and well known results of the theory of special relativity. However, most of the corresponding notations used either in astrophysics or in statistical physics are rather unusual. Therefore a few words about these notations can be useful even for some advanced readers.

Keywords

Fermi Level Neutron Star Energy Parameter Elementary Property Occupancy Rate 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Chandrasekhar, S.: 1939, An Introduction to the Study of Stellar Structure, Univ. of Chicago Press. (Reprinted 1967), Dover, New York).Google Scholar
  2. Kittel, C.: 1969, Thermal Physics, Wiley, New York.Google Scholar
  3. Kittel, C., Knight, W. D., Ruderman, M. A.: 1962, Mechanics (Berkeley Physics Course, Vol. I), McGraw-Hill, New York.Google Scholar
  4. Reif, F.: 1964, Statistical Physics (Berkeley Physics Course, Vol. V), (Section 3.5 (p. 121)), McGraw-Hill, New York.Google Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1980

Authors and Affiliations

  • V. Kourganoff
    • 1
  1. 1.University of ParisFrance

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