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dc.date.accessioned 2019-10-02T12:43:04Z
dc.date.available 2019-10-02T12:43:04Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82455
dc.description.abstract We study the Brown-York quasilocal energy for regular black holes. We also express the identity that relates the difference of the Brown-York quasilocal energy and the Komar charge at the horizon to the total energy of the spacetime for static and spherically symmetric black hole solutions in a convenient way which permits us to understand why this identity is not satisfied when we consider nonlinear electrodynamics. However, we give a relation between quantities evaluated at the horizon and at infinity when nonlinear electrodynamics is considered. Similar relations are obtained for more general static and spherically symmetric black hole solutions which include solutions of dilaton gravity theories. en
dc.format.extent 280-285 es
dc.language en es
dc.subject Black hole horizon es
dc.subject Quasilocal energy es
dc.subject Regular black holes es
dc.title Quasilocal energy, Komar charge and horizon for regular black holes en
dc.type Articulo es
sedici.identifier.other eid:2-s2.0-77950298765 es
sedici.identifier.other doi:10.1016/j.physletb.2010.03.056 es
sedici.identifier.issn 03702693 es
sedici.creator.person Balart Vergara, Leonardo es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physics Letters B es
sedici.relation.journalVolumeAndIssue vol. 687, no. 4-5 es


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