Logarithmic correction to BH entropy as Noether charge

dc.contributor.authorAros, R.
dc.contributor.authorDíaz, D.E.
dc.contributor.authorMontecinos, A.
dc.date.accessioned2013-10-22T18:50:36Z
dc.date.accessioned2016-05-24T20:18:58Z
dc.date.available2013-10-22T18:50:36Z
dc.date.available2016-05-24T20:18:58Z
dc.date.issued2010
dc.descriptionIndexación: Springer
dc.description.abstractWe consider the role of the type-A trace anomaly in static black hole solutions to semiclassical Einstein equations in four dimensions. Via Wald’s Noether charge formalism, we compute the contribution to the entropy coming from the anomaly induced effective action and unveil a logarithmic correction to the Bekenstein-Hawking area law. The corrected entropy is given by a seemingly universal formula Sbh = AH 4 − a · χH · φH involving the coefficient a of the type-A trace anomaly, the Euler characteristic χH of the horizon and the value at the horizon φH of the solution to the uniformization problem for Q-curvature. Two instances are examined in detail: Schwarzschild and a four-dimensional massless topological black hole. We also find agreement with the logarithmic correction due to one-loop contribution of conformal fields in the Schwarzschild background.en
dc.description.urihttp://www.springerlink.com/content/1781827x318218r1/fulltext.pdf
dc.identifier.citationJournal of high energy physics, vol. 7, 2010.
dc.identifier.otherDOI: 10.1007/JHEP07(2010)012
dc.identifier.urihttp://repositorio.unab.cl/xmlui/handle/ria/1933
dc.language.isoen
dc.publisherSpringer Verlag
dc.rights.holderSpringer
dc.subjectBlack Holes
dc.subjectAnomalies in Field
dc.subjectString Theories
dc.titleLogarithmic correction to BH entropy as Noether charge
dc.typeArtículo
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