2008
DOI: 10.1002/prop.200810565
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Universal Kounterterms in Lovelock AdS gravity

Abstract: We show the universal form of the boundary term (Kounterterm series) which regularizes the Euclidean action and background-independent definition of conserved quantities for any Lovelock gravity theory with AdS asymptotics (including Einstein-Hilbert and Einstein-Gauss-Bonnet). We discuss on the connection of this procedure to the existence of topological invariants and ChernSimons forms in the corresponding dimensions.

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Cited by 26 publications
(33 citation statements)
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“…Not surprisingly, this is the case. Expanding the contractions of the Weyl tensor, 11) and using the fact that the Weyl tensor is traceless, we can show that…”
Section: Jhep11(2017)128mentioning
confidence: 99%
“…Not surprisingly, this is the case. Expanding the contractions of the Weyl tensor, 11) and using the fact that the Weyl tensor is traceless, we can show that…”
Section: Jhep11(2017)128mentioning
confidence: 99%
“…As shown in [78,79], the LL AdS action is regularized by the same boundary term as the one in Einstein-Hilbert or EGB gravity with negative cosmological constant in even or odd dimensions, which is known to be universal for any Lovelock gravity. The only quantity that changes is the coefficient c d , which depends on eff as one of the roots of the polynomial (7).…”
Section: Free Energy Of a Lovelock Superconductor In Canonical And Grmentioning
confidence: 95%
“…An advantage of this procedure is that the boundary term is well known for any LL gravity in any dimension because its form is universal, of a geometric origin [78,79]. Additionally, it is background independent, covariant and in Fefferman-Graham coordinates gives the results consistent with the holographic renormalization [80], in cases when the last one can be done explicitly.…”
Section: Variational Principle and Boundary Termsmentioning
confidence: 96%
“…In even dimensions D = 2n > 4, I E has to be supplemented by the n-th Chern form B E 1 with the fixed coefficient. 13 For the matter fields, we can choose the boundary term that does not modify the black hole mass,…”
Section: Free Energymentioning
confidence: 99%