Horizon thermalization of Kerr black hole through local instability

DOI10.1016/j.physletb.2022.136899zbMath1486.83099arXiv2103.11613OpenAlexW3139403273MaRDI QIDQ2076674

Surojit Dalui, Bibhas Ranjan Majhi

Publication date: 22 February 2022

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2103.11613

Mathematics Subject Classification ID

Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (2)

Quantum corrections enhance chaos: study of particle motion near a generalized Schwarzschild black hole ⋮ BMS Goldstone modes near the horizon of a Kerr black hole are thermal

Cites Work

• Particle creation by black holes
• The black hole S-matrix from quantum mechanics
• Physics of the inverted harmonic oscillator: From the lowest Landau level to event horizons
• Thermalization of horizon through asymptotic symmetry in three-dimensional massive gravity
• The four laws of black hole mechanics
• Gravitation
• Hawking Radiation As Tunneling
• Black Holes and Entropy
• Black hole explosions?

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