Computing Black Hole entropy in Loop Quantum Gravity from a Conformal Field Theory perspective
arXiv:0903.1667 · doi:10.1088/1475-7516/2009/07/016
Abstract
Motivated by the analogy proposed by Witten between Chern-Simons and Conformal Field Theories, we explore an alternative way of computing the entropy of a black hole starting from the isolated horizon framework in Loop Quantum Gravity. The consistency of the result opens a window for the interplay between Conformal Field Theory and the description of black holes in Loop Quantum Gravity.
9 pages
References in corpus (4)
Cited by in corpus (5)
- Black Holes in Loop Quantum Gravity
- Detailed black hole state counting in loop quantum gravity
- The combinatorics of the SU(2) black hole entropy in loop quantum gravity
- Isolated Horizons and Black Hole Entropy in Loop Quantum Gravity
- Acceleration radiation, transition probabilities, and trans-Planckian physics