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

2000/06/16 by Carlos Pinheiro, Pinheiro, Carlos, F. C. Khanna +1
Physics and Astronomy · #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Theory (hep-th) #gr-qc #hep-th

paper · pdf · doi:10.48550/arxiv.hep-th/0006131

8 pages, LaTex

arxiv created 2000/06/16 · arxiv updated 2009/11/30

Abstract

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.

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