Thermodynamics of noncommutative quantum Kerr black holes
arXiv:1602.05989 · doi:10.3390/e18110406
Abstract
Thermodynamic formalism for rotating black holes, characterized by noncommutative and quantum corrections, is constructed. From a fundamental thermodynamic relation, equations of state and thermodynamic response functions are explicitly given and the effect of noncommutativity and quantum correction is discussed. It is shown that the well known divergence exhibited in specific heat is not removed by any of these corrections. However, regions of thermodynamic stability are affected by noncommutativity, increasing the available states for which some thermodynamic stability conditions are satisfied.
arXiv comment16 pages, 9 figures
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- Noncommutative cosmological models induced by a symplectic formalism coupled to phantom fluids
- Coalescence of Kerr Black Holes: Binary Systems from GW150914 to GW170814
- Corrections to the Black hole entropy from a Bose Einstein condensate: a semi-classical phenomenological approach