Non-extensive statistics and the stellar polytrope index
Within the domain of a classical non-extensive kinetic theory, we use physical constrains imposed by the H-theorem and by the negative nature of the heat capacity of self-gravitating thermodynamically isolated systems to investigate some possible limits on the stellar polytrope index n.
Year of publication: |
2004
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Authors: | Silva, R ; Alcaniz, J.S |
Published in: |
Physica A: Statistical Mechanics and its Applications. - Elsevier, ISSN 0378-4371. - Vol. 341.2004, C, p. 208-214
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Publisher: |
Elsevier |
Subject: | Non-extensive statistic | Stellar polytrope | Kinetic theory |
Saved in:
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