Elementary Properties of a Degenerate Fermi Gas
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.
KeywordsFermi Level Neutron Star Energy Parameter Elementary Property Occupancy Rate
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- Chandrasekhar, S.: 1939, An Introduction to the Study of Stellar Structure, Univ. of Chicago Press. (Reprinted 1967), Dover, New York).Google Scholar
- Kittel, C.: 1969, Thermal Physics, Wiley, New York.Google Scholar
- Kittel, C., Knight, W. D., Ruderman, M. A.: 1962, Mechanics (Berkeley Physics Course, Vol. I), McGraw-Hill, New York.Google Scholar
- Reif, F.: 1964, Statistical Physics (Berkeley Physics Course, Vol. V), (Section 3.5 (p. 121)), McGraw-Hill, New York.Google Scholar