Truncated Heat Kernel and One-Loop Determinants for the BTZ Geometry

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dc.creatorBytsenko, A. A.
dc.creatorGuimaraes, M. E. X.
dc.date2008-09-08
dc.date.accessioned2026-07-07T12:15:35Z
dc.date.available2026-07-07T12:15:35Z
dc.descriptionThere is a special relation between the spectrum and the {\it truncated} heat kernel of the Euclidean BTZ black hole with the Patterson-Selberg zeta function. Using an orbifold description of this relation we calculate the on-shell corrections of the gravitational quantum fluctuations.
dc.description10 pages. To appear in the European Phys. J. C
dc.identifierhttps://arxiv.org/abs/0809.1416
dc.identifierhttp://arxiv.org/abs/0809.1416
dc.identifierEur.Phys.J.C58:511-516,2008
dc.identifierdoi:10.1140/epjc/s10052-008-0743-y
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211532
dc.subjectHigh Energy Physics - Theory
dc.titleTruncated Heat Kernel and One-Loop Determinants for the BTZ Geometry
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