Instabilities of naked singularities and black hole interiors in General Relativity

Metrics representing black holes in General Relativity may exhibit naked singularities for certain values of their parameters. This is the case for super-extremal (J2 > M > 0) Kerr and super-extremal (|Q| > M > 0) Reissner-Nordstrom spacetimes, and also for the negative mass Schwarzschil...

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Detalles Bibliográficos
Autores principales:	Dotti, Gustavo, Gleiser, Reinaldo J., Pullin, Jorge, Ranea Sandoval, Ignacio Francisco, Vucetich, Héctor
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2009
Materias:	Física Astronomía Einstein gravity Naked singularities Black hole interiors Stability
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/129268
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

id	I19-R120-10915-129268
record_format	dspace
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Física Astronomía Einstein gravity Naked singularities Black hole interiors Stability
spellingShingle	Física Astronomía Einstein gravity Naked singularities Black hole interiors Stability Dotti, Gustavo Gleiser, Reinaldo J. Pullin, Jorge Ranea Sandoval, Ignacio Francisco Vucetich, Héctor Instabilities of naked singularities and black hole interiors in General Relativity
topic_facet	Física Astronomía Einstein gravity Naked singularities Black hole interiors Stability
description	Metrics representing black holes in General Relativity may exhibit naked singularities for certain values of their parameters. This is the case for super-extremal (J2 > M > 0) Kerr and super-extremal (\|Q\| > M > 0) Reissner-Nordstrom spacetimes, and also for the negative mass Schwarzschild spacetime. We review our recent work where we show that these nakedly singular spacetimes are unstable under linear gravitational perturbations, a result that supports the cosmic censorship conjecture, and also that the inner stationary region beyond the inner horizon of a Kerr black hole (J2 < M) is linearly unstable.
format	Articulo Preprint
author	Dotti, Gustavo Gleiser, Reinaldo J. Pullin, Jorge Ranea Sandoval, Ignacio Francisco Vucetich, Héctor
author_facet	Dotti, Gustavo Gleiser, Reinaldo J. Pullin, Jorge Ranea Sandoval, Ignacio Francisco Vucetich, Héctor
author_sort	Dotti, Gustavo
title	Instabilities of naked singularities and black hole interiors in General Relativity
title_short	Instabilities of naked singularities and black hole interiors in General Relativity
title_full	Instabilities of naked singularities and black hole interiors in General Relativity
title_fullStr	Instabilities of naked singularities and black hole interiors in General Relativity
title_full_unstemmed	Instabilities of naked singularities and black hole interiors in General Relativity
title_sort	instabilities of naked singularities and black hole interiors in general relativity
publishDate	2009
url	http://sedici.unlp.edu.ar/handle/10915/129268
work_keys_str_mv	AT dottigustavo instabilitiesofnakedsingularitiesandblackholeinteriorsingeneralrelativity AT gleiserreinaldoj instabilitiesofnakedsingularitiesandblackholeinteriorsingeneralrelativity AT pullinjorge instabilitiesofnakedsingularitiesandblackholeinteriorsingeneralrelativity AT raneasandovalignaciofrancisco instabilitiesofnakedsingularitiesandblackholeinteriorsingeneralrelativity AT vucetichhector instabilitiesofnakedsingularitiesandblackholeinteriorsingeneralrelativity
bdutipo_str	Repositorios
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Instabilities of naked singularities and black hole interiors in General Relativity

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