Stress-Energy Tensors for Higher Dimensional Gravity

dc.creatorDeBenedictis, A.
dc.creatorViswanathan, K. S.
dc.date1999-11-09
dc.date.accessioned2026-07-07T04:27:17Z
dc.date.available2026-07-07T04:27:17Z
dc.descriptionWe calculate, in the context of higher dimensional gravity, the stress-energy tensor and Weyl anomaly associated with anti-de Sitter and anti-de Sitter black hole solutions. The boundary counter-term method is used to regularize the action and the resulting stress-energy tensor yields both the correct black hole energies as well as a vacuum energy contribution which is interpreted as a Casimir energy. This calculation is done up to d = 8 (d being the boundary dimension). We confirm some results for d < 8 as well as comment on some new results (some of which are relevant to (2,0) theory). All results for d=8 are new.
dc.description12 pages. Uses AMS package. No figures
dc.identifierhttps://arxiv.org/abs/hep-th/9911060
dc.identifierhttp://arxiv.org/abs/hep-th/9911060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/56366
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStress-Energy Tensors for Higher Dimensional Gravity
dc.typetext

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