On the thermodynamic stability of rotating black holes in higher dimensions—a comparision of thermodynamic ensembles

DOI10.1088/0264-9381/31/13/135012zbMath1298.83077arXiv1312.6810OpenAlexW3104398582MaRDI QIDQ2874792

Brian P. Dolan

Publication date: 8 August 2014

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1312.6810

zbMATH Keywords

stability analysisrotationthermodynamicsblack holeshigher dimensionsMyers-Perry black hole

Mathematics Subject Classification ID

Geometric invariant theory (14L24) Black holes (83C57) Vector and tensor algebra, theory of invariants (15A72) Entropy and other invariants (28D20) Eigenvalues, singular values, and eigenvectors (15A18) Classical and relativistic thermodynamics (80A10) Kaluza-Klein and other higher-dimensional theories (83E15) Actions of groups on commutative rings; invariant theory (13A50) Canonical forms, reductions, classification (15A21)

Related Items (4)

\(P\) - \(v\) criticality in quasitopological gravity ⋮ Thermodynamic volume of cosmological solitons ⋮ Thermodynamical stability of \(f(R)\)-AdS black holes in grand canonical ensemble ⋮ Reverse Hawking-Page phase transition in de Sitter black holes

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