http://arxiv.org/abs/1411.0325
The conditions for thermal equilibrium given in [Class. Quantum Grav. 30 115018 (2013)] are outlined. It is also clarified that the condition for the equivalence between thermodynamic and dynamical stability of static spherically symmetric perfect fluids in General Relativity was referring to the canonical ensemble. Cases for which stability equivalence holds are specified.
Z. Roupas
Tue, 4 Nov 14
3/76
Comments: 4 pages
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