‘Quantum hairs’ and entropy of the quantum isolated horizon from Chern–Simons theory

DOI10.1088/0264-9381/31/19/195003zbMath1319.83014arXiv1301.4553OpenAlexW3106531827WikidataQ113390351 ScholiaQ113390351MaRDI QIDQ2930666

Abhishek Majhi, Parthasarathi Majumdar

Publication date: 19 November 2014

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

Full work available at URL: https://arxiv.org/abs/1301.4553

zbMATH Keywords

entropyblack holequantum isolated horizonquantum hairstatisical mechanics

Mathematics Subject Classification ID

Black holes (83C57) Classical equilibrium statistical mechanics (general) (82B05) Quantization of the gravitational field (83C45) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Measures of information, entropy (94A17) Eta-invariants, Chern-Simons invariants (58J28)

Related Items (7)

Black hole entropy from indistinguishable quantum geometric excitations ⋮ Conformal blocks on a 2-sphere with indistinguishable punctures and implications on black hole entropy ⋮ Energy spectrum of black holes: A new view ⋮ Thermal stability of black holes with arbitrary hairs ⋮ Note on SU(2) isolated horizon ⋮ Quasi stable black holes and their implications ⋮ Thermal stability of charged rotating quantum black holes

This page was built for publication: ‘Quantum hairs’ and entropy of the quantum isolated horizon from Chern–Simons theory