Thermal stability of black holes with arbitrary hairs

DOI10.1142/S0217732318500311zbMath1382.83070arXiv1702.08175WikidataQ113388109 ScholiaQ113388109MaRDI QIDQ4608175

Aloke Kumar Sinha

Publication date: 16 March 2018

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1702.08175

zbMATH Keywords

quantum gravitythermal stabilityquantum black hole

Mathematics Subject Classification ID

Black holes (83C57) Quantum equilibrium statistical mechanics (general) (82B10)

Related Items (2)

Dying AdS Schwarzschild black hole ⋮ Quasi stable black holes and their implications

Cites Work

• Black holes in higher dimensional space-times
• Isolated and dynamical horizons and their applications
• Charged quantum black holes: thermal stability criterion
• ‘Quantum hairs’ and entropy of the quantum isolated horizon from Chern–Simons theory
• Black holes in magnetic monopoles
• Thermal stability of charged rotating quantum black holes
• Generalized Hawking–Page phase transition
• Quantum hair
• Colored black holes
• Growing hair on black holes
• Quantum Geometry and Black Hole Entropy
• Dilaton black holes with a cosmological term
• Modern Canonical Quantum General Relativity
• Quantum Gravity
• Quantum geometry of isolated horizons and black hole entropy

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