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dc.creatorGallo, Emanuel-
dc.creatorVillanueva, Jose R.-
dc.date2018-07-05T17:34:31Z-
dc.date2018-07-05T17:34:31Z-
dc.date2015-09-
dc.date2018-07-03T21:52:33Z-
dc.date.accessioned2019-04-29T15:46:37Z-
dc.date.available2019-04-29T15:46:37Z-
dc.date.issued2015-09-
dc.identifierGallo, Emanuel; Villanueva, Jose R.; Photon spheres in Einstein and Einstein-Gauss-Bonnet theories and circular null geodesics in axially-symmetric spacetimes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 92; 6; 9-2015-
dc.identifier1550-7998-
dc.identifierhttp://hdl.handle.net/11336/51365-
dc.identifier1550-2368-
dc.identifierCONICET Digital-
dc.identifierCONICET-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/301720-
dc.descriptionIn this article we extend a recent theorem proven by Hod [Upper bound on the radii of black-hole photon spheres, Phys. Lett. B 727, 345 (2013)] to n-dimensional Einstein and Einstein-Gauss-Bonnet theories, which gives an upper bound for the photon sphere radii of spherically symmetric black holes. As applications of these results we give a universal upper bound for the real part of quasinormal modes in the WKB limit and a universal lower bound for the position of the first relativistic image in the strong lensing regime produced by these type of black holes. For the axially-symmetric case, we also make some general comments (independent of the underlying gravitational theory) on the relation between circular null geodesics and the fastest way to circle a black hole.-
dc.descriptionFil: Gallo, Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Física Enrique Gaviola. Universidad Nacional de Córdoba. Instituto de Física Enrique Gaviola; Argentina. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina-
dc.descriptionFil: Villanueva, Jose R.. Universidad de Valparaíso. Instituto de Física y Astronomía; Chile. Centro de Astrofísica de Valparaíso; Chile-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherAmerican Physical Society-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevD.92.064048-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.92.064048-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.subjectBLACK HOLES-
dc.subjectQUASI-NORMAL MODES-
dc.subjectPHOTON SPHERES-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titlePhoton spheres in Einstein and Einstein-Gauss-Bonnet theories and circular null geodesics in axially-symmetric spacetimes-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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