On the linear stability of the extreme Kerr black hole under axially symmetric perturbations

dc.creatorDain, Sergio Alejandro
dc.creatorGentile de Austria, Ivan
dc.date.accessioned2017-12-28T17:34:31Z
dc.date.accessioned2018-11-06T15:46:05Z
dc.date.available2017-12-28T17:34:31Z
dc.date.available2018-11-06T15:46:05Z
dc.date.created2017-12-28T17:34:31Z
dc.date.issued2014-09
dc.identifierGentile de Austria, Ivan; Dain, Sergio Alejandro; On the linear stability of the extreme Kerr black hole under axially symmetric perturbations; IOP Publishing; Classical and Quantum Gravity; 31; 19; 9-2014
dc.identifier0264-9381
dc.identifierhttp://hdl.handle.net/11336/31826
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1900796
dc.description.abstractWe prove that for axially symmetric linear gravitational perturbations of the extreme Kerr black hole, there exists a positive definite and conserved energy. This provides a basic criteria for linear stability in axial symmetry. In the particular case of Minkowski, using this energy we also prove the pointwise boundedness of the perturbation in a remarkably simple way.
dc.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0264-9381/31/19/195009
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0264-9381/31/19/195009/meta
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectLINEAR
dc.subjectSTABILITY
dc.subjectKERR
dc.subjectPERTURBATIONS
dc.titleOn the linear stability of the extreme Kerr black hole under axially symmetric perturbations
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


Este ítem pertenece a la siguiente institución