Topological invariants and the definition of energy in quadratic gravity theory

dc.creatorG, Giribet
dc.creatorO, Miskovic
dc.creatorOlea, R
dc.creatorRivera Betancour, D
dc.date.accessioned2021-07-23T15:10:40Z
dc.date.accessioned2024-05-02T15:03:29Z
dc.date.available2021-07-23T15:10:40Z
dc.date.available2024-05-02T15:03:29Z
dc.date.created2021-07-23T15:10:40Z
dc.date.issued2020-03
dc.identifierPhysical Review D Open AccessVolume 101, Issue 615 March 2020 Article number 064046
dc.identifier24700010
dc.identifierhttp://repositorio.unab.cl/xmlui/handle/ria/19482
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9261642
dc.description.abstractAbstract We provide a simple method to compute the energy in higher curvature gravity in asymptotically AdS spacetimes in even dimensions. It follows from the combined use of topological terms added to the gravity action, and the Wald charges derived from the augmented action functional. No additional boundary terms are needed. As a consistency check, we show that the formula for the conserved quantities derived in this way yields the correct result for the mass of asymptotically AdS black holes. © 2020 authors. Published by the American Physical Society. Learn about these Topics
dc.languageen
dc.publisherAmerican Physical Society
dc.subjectBlack Holes; Event Horizon; Supergravity
dc.titleTopological invariants and the definition of energy in quadratic gravity theory
dc.typeArtículo


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