Vacuum energy in asymptotically flat 2 + 1 gravity

dc.contributor.authorMiskovic, Olivera
dc.contributor.authorOlea, Rodrigo
dc.contributor.authorRoy, Debraj
dc.date.accessioned2024-06-18T19:09:03Z
dc.date.available2024-06-18T19:09:03Z
dc.date.issued2017-04
dc.descriptionIndexación: Scopus
dc.description.abstractWe compute the vacuum energy of three-dimensional asymptotically flat space based on a Chern–Simons formulation for the Poincaré group. The equivalent action is nothing but the Einstein–Hilbert term in the bulk plus half of the Gibbons–Hawking term at the boundary. The derivation is based on the evaluation of the Noether charges in the vacuum. We obtain that the vacuum energy of this space has the same value as the one of the asymptotically flat limit of three-dimensional anti-de Sitter space. © 2017 The Author(s)
dc.description.urihttps://www.sciencedirect.com/science/article/pii/S0370269317300965?via%3Dihub
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics Volume 767, Pages 258 - 26310 April 2017
dc.identifier.doi10.1016/j.physletb.2017.02.006
dc.identifier.issn0370-2693
dc.identifier.urihttps://repositorio.unab.cl/handle/ria/57737
dc.language.isoen
dc.publisherElsevier B.V.
dc.rights.licenseATRIBUCIÓN 4.0 INTERNACIONAL CC BY 4.0 Deed
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/deed.es
dc.titleVacuum energy in asymptotically flat 2 + 1 gravity
dc.typeArtículo
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