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dc.date.accessioned 2020-06-03T16:21:41Z
dc.date.available 2020-06-03T16:21:41Z
dc.date.issued 2013-10-25
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/97411
dc.description.abstract We analyze the thermodynamical properties of the regular static and spherically symmetric black hole interior model presented by Mbonye and Kazanas. Equations for the thermodynamical quantities valid for an arbitrary density profile are deduced, and from them we show that the model is thermodynamically unstable. Evidence is also presented pointing to its dynamical instability. The gravitational entropy of this solution based on the Weyl curvature conjecture is calculated, following the recipe given by Rudjord, Grøn and Sigbjørn, and it is shown to have the expected behavior. en
dc.format.extent 734-753 es
dc.language en es
dc.subject Black holes es
dc.subject General relativity es
dc.subject Thermodynamics es
dc.subject Gravitational entropy es
dc.title An analysis of a regular black hole interior model en
dc.type Articulo es
sedici.identifier.uri https://ri.conicet.gov.ar/11336/5836 es
sedici.identifier.uri http://link.springer.com/article/10.1007/s10773-013-1861-3 es
sedici.identifier.uri http://arxiv.org/abs/1111.0690v2 es
sedici.identifier.other arXiv:1111.0690v2 es
sedici.identifier.other http://dx.doi.org/10.1007/s10773-013-1861-3 es
sedici.identifier.other hdl:11336/5836 es
sedici.identifier.issn 0020-7748 es
sedici.creator.person Pérez, Daniela es
sedici.creator.person Romero, Gustavo Esteban es
sedici.creator.person Pérez Bergliaffa, Santiago Esteban es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Preprint 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 International Journal of Theoretical Physics es
sedici.relation.journalVolumeAndIssue vol. 53, no. 3 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)