Energy in Generic Higher Curvature Gravity Theories

dc.creatorDeser, S.
dc.creatorTekin, Bayram
dc.date2002-12-23
dc.date2003-01-24
dc.date.accessioned2026-07-07T11:48:04Z
dc.date.available2026-07-07T11:48:04Z
dc.descriptionWe define and compute the energy of higher curvature gravity theories in arbitrary dimensions. Generically, these theories admit constant curvature vacua (even in the absence of an explicit cosmological constant), and asymptotically constant curvature solutions with non-trivial energy properties. For concreteness, we study quadratic curvature models in detail. Among them, the one whose action is the square of the traceless Ricci tensor always has zero energy, unlike conformal (Weyl) gravity. We also study the string-inspired Einstein-Gauss-Bonnet model and show that both its flat and Anti-de-Sitter vacua are stable.
dc.description18 pages, typos corrected, one footnote added, to appear in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/hep-th/0212292
dc.identifierhttp://arxiv.org/abs/hep-th/0212292
dc.identifierPhys.Rev.D67:084009,2003
dc.identifierdoi:10.1103/PhysRevD.67.084009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202793
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEnergy in Generic Higher Curvature Gravity Theories
dc.typetext

Files

Collections