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Negative heat capacity and non-extensive kinetic theory

arXiv:astro-ph/0306009 · doi:10.1016/S0375-9601(03)00858-2

Abstract

The negative nature of the heat capacity $C_V$ of thermodynamically isolated self-gravitating systems is rediscussed in the framework of a non-extensive kinetic theory. It is found that the dependence of $C_V$ on the non-extensive parameter $q$ gives rise to a negative branch with the critical value corresponding to $q = 5/3$ ($C_V\to - \infty$).

7 pages, 1 figure, revised version to appear in Phys. Lett. A