Thermal stability of charged rotating quantum black holes

DOI10.1142/S021773231750208XzbMath1378.83047arXiv1512.04181OpenAlexW2770536661MaRDI QIDQ3130374

Parthasarathi Majumdar, Aloke Kumar Sinha

Publication date: 22 January 2018

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

Full work available at URL: https://arxiv.org/abs/1512.04181

zbMATH Keywords

loop quantum gravitythermal stabilityquantum black hole

Mathematics Subject Classification ID

Black holes (83C57) Gravitational interaction in quantum theory (81V17)

Related Items (4)

Resolving the information loss paradox from the five-dimensional minimal supergravity black hole ⋮ Dying AdS Schwarzschild black hole ⋮ Thermal stability of black holes with arbitrary hairs ⋮ Quasi stable black holes and their implications

Cites Work

• Isolated and dynamical horizons and their applications
• Modelling black holes with angular momentum in loop quantum gravity
• Charged quantum black holes: thermal stability criterion
• ‘Quantum hairs’ and entropy of the quantum isolated horizon from Chern–Simons theory
• Generalized Hawking–Page phase transition
• Rotating charged black hole solution in heterotic string theory
• Quantum Geometry and Black Hole Entropy
• Thermodynamics of Kerr-Newman-AdS black holes and conformal field theories
• Modern Canonical Quantum General Relativity
• Quantum Gravity
• Quantum geometry of isolated horizons and black hole entropy

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