Black Hole Entropy in 1+1 Dimensions from a Quasi-Chern Simons term in a Gravitational Background

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We introduce a 'quasi-topological` term [1] in D=1+1 dimensions and the entropy for black holes is calculated [2]. The source of entropy in this case is justified by a non-null stress-energy tensor.
8 pages, LaTex

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High Energy Physics - Theory, General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/50075

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/hep-th/0006131
 http://arxiv.org/abs/hep-th/0006131

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arXiv