Mass and horizon Dirac observables in effective models of quantum black-to-white hole transition
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Publication:5163354
DOI10.1088/1361-6382/abe05dzbMath1483.83022arXiv1912.00774OpenAlexW3144609016MaRDI QIDQ5163354
Fabio M. Mele, Johannes Münch, Norbert Bodendorfer
Publication date: 3 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1912.00774
Black holes (83C57) Statistical mechanics of polymers (82D60) Quantization of the gravitational field (83C45)
Related Items (13)
Quantum corrected polymer black hole thermodynamics: mass relations and logarithmic entropy correction ⋮ Bouncing compact objects. Part I. Quantum extension of the Oppenheimer-Snyder collapse ⋮ A consistent model of non-singular Schwarzschild black hole in loop quantum gravity and its quasinormal modes ⋮ Towards consistent black-to-white hole bounces from matter collapse ⋮ Regular black holes: a short topic review ⋮ On the horizon area of effective loop quantum black holes ⋮ Generic features of a polymer quantum black hole ⋮ Probing effective loop quantum gravity on weak gravitational lensing, Hawking radiation and bounding greybody factor by black holes ⋮ Remnant loop quantum black holes ⋮ \((b,v)\)-type variables for black to white hole transitions in effective loop quantum gravity ⋮ Effective quantum dust collapse via surface matching ⋮ Destroying the event horizon of a nonsingular rotating quantum-corrected black hole ⋮ Loop Quantum Gravity motivated multihorizon rotating black holes
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