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Entropy 2012, 14(6), 1045-1078; doi:10.3390/e14061045

Thermodynamic Geometry and Topological Einstein–Yang–Mills Black Holes

INFN-Laboratori Nazionali di Frascati, Via E. Fermi 40, 00044 Frascati, Italy
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Received: 25 April 2012 / Revised: 8 June 2012 / Accepted: 11 June 2012 / Published: 13 June 2012
(This article belongs to the Special Issue Black Hole Thermodynamics)
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Abstract

From the perspective of the statistical fluctuation theory, we explore the role of the thermodynamic geometries and vacuum (in)stability properties for the topological Einstein–Yang–Mills black holes. In this paper, from the perspective of the state-space surface and chemical Weinhold surface of higher dimensional gravity, we provide the criteria for the local and global statistical stability of an ensemble of topological Einstein–Yang–Mills black holes in arbitrary spacetime dimensions D ≥ 5. Finally, as per the formulations of the thermodynamic geometry, we offer a parametric account of the statistical consequences in both the local and global fluctuation regimes of the topological extremal Einstein–Yang–Mills black holes. View Full-Text
Keywords: thermodynamic geometry; topological Einstein–Yang–Mills black holes; higher dimensional gravity; cosmological constant thermodynamic geometry; topological Einstein–Yang–Mills black holes; higher dimensional gravity; cosmological constant
This is an open access article distributed under the Creative Commons Attribution License (CC BY 3.0).

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Bellucci, S.; Tiwari, B.N. Thermodynamic Geometry and Topological Einstein–Yang–Mills Black Holes. Entropy 2012, 14, 1045-1078.

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