Non-extensive statistics and the stellar polytrope index

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages, 2 figures, LaTeX

Scientific paper

10.1016/j.physa.2004.02.070

We use physical constrains imposed from the H-Theorem and from the negative
nature of the heat capacity of self-gravitating thermodynamically isolated
systems to investigate some possible limits on the stellar polytrope index $n$
within the domain of a classical non-extensive kinetic theory.

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