Counting black hole microscopic states in loop quantum gravity
arXiv:hep-th/0605125 · doi:10.1103/PhysRevD.74.064026
Abstract
Counting of microscopic states of black holes is performed within the framework of loop quantum gravity. This is the first calculation of the pure horizon states using statistical methods, which reveals the possibility of additional states missed in the earlier calculations, leading to an increase of entropy. Also for the first time a microcanonical temperature is introduced within the framework.
5 pages, revtex: version to appear in PRD
Cited by in corpus (6)
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- Toward explaining black hole entropy quantization in loop quantum gravity
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- Considering boundary conditions for black hole entropy in loop quantum gravity