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

Simple item page
dc.creatorPinheiro, Carlos
dc.creatorKhanna, F. C.
dc.date2000-06-16
dc.date.accessioned2026-07-07T04:10:00Z
dc.date.available2026-07-07T04:10:00Z
dc.descriptionWe 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.
dc.description8 pages, LaTex
dc.identifierhttps://arxiv.org/abs/hep-th/0006131
dc.identifierhttp://arxiv.org/abs/hep-th/0006131
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50075
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Hole Entropy in 1+1 Dimensions from a Quasi-Chern Simons term in a Gravitational Background
dc.typetext

Files

Collections

arXiv