Holography with Gravitational Chern-Simons Term

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dc.creatorSolodukhin, Sergey N.
dc.date2005-09-20
dc.date2005-12-28
dc.date.accessioned2026-07-07T10:30:18Z
dc.date.available2026-07-07T10:30:18Z
dc.descriptionThe holographic description in the presence of gravitational Chern-Simons term is studied. The modified gravitational equations are integrated by using the Fefferman-Graham expansion and the holographic stress-energy tensor is identified. The stress-energy tensor has both conformal anomaly and gravitational or, if re-formulated in terms of the zweibein, Lorentz anomaly. We comment on the structure of anomalies in two dimensions and show that the two-dimensional stress-energy tensor can be reproduced by integrating the conformal and gravitational anomalies. We study the black hole entropy in theories with a gravitational Chern-Simons term and find that the usual Bekenstein-Hawking entropy is modified. For the BTZ black hole the modification is determined by area of the inner horizon. We show that the total entropy of the BTZ black hole is precisely reproduced in a boundary CFT calculation using the Cardy formula.
dc.description19 pages, Latex; v3: minor corrections, some clarifications
dc.identifierhttps://arxiv.org/abs/hep-th/0509148
dc.identifierhttp://arxiv.org/abs/hep-th/0509148
dc.identifierPhys.Rev.D74:024015,2006
dc.identifierdoi:10.1103/PhysRevD.74.024015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178092
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectDifferential Geometry
dc.titleHolography with Gravitational Chern-Simons Term
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