Dolan, Brian P.
(2014)
Thermodynamic stability of asymptotically
anti-de Sitter rotating black holes in higher
dimensions.
Classical and Quantum Gravity, 31 (165011).
pp. 1-23.
ISSN 0264-9381
Abstract
Conditions for thermodynamic stability of asymptotically anti-de Sitter rotating
black holes in D-dimensions are determined. Local thermodynamic
stability requires not only positivity conditions on the specific heat and the
moment of inertia tensor but it is also necessary that the adiabatic compressibility
be positive. It is shown that, in the absence of a cosmological constant,
neither rotation nor charge is sufficient to ensure full local thermodynamic
stability of a black hole.
Thermodynamic stability properties of anti-de Sitter Myers-Perry black
holes are investigated for both singly spinning and multi-spinning black holes.
Simple expressions are obtained for the specific heat and moment of inertia
tensor in any dimension. An analytic expression is obtained for the boundary
of the region of parameter space in which such space-times are thermodynamically
stable.
Item Type: |
Article
|
Additional Information: |
Postprint version of published article. The definitive version of this article is available at Thermodynamic stability of asymptotically anti-de Sitter rotating black holes in higher dimensions; Brian P Dolan 2014 Class. Quantum Grav. 31 165011 DOI: 10.1088/0264-9381/31/16/165011 |
Keywords: |
black holes; higher dimensions; anti-de Sitter; rotation; thermodynamics; |
Academic Unit: |
Faculty of Science and Engineering > Mathematical Physics |
Item ID: |
5819 |
Identification Number: |
https://doi.org/10.1088/0264-9381/31/16/165011 |
Depositing User: |
Dr. Brian Dolan
|
Date Deposited: |
11 Feb 2015 15:02 |
Journal or Publication Title: |
Classical and Quantum Gravity |
Publisher: |
Institute of Physics |
Refereed: |
Yes |
URI: |
|
Use Licence: |
This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available
here |
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