Extremal black hole initial data deformations

dc.creatorAceña, Andrés Esteban
dc.creatorGabach Clement, Maria Eugenia
dc.date.accessioned2020-03-20T18:26:06Z
dc.date.accessioned2022-10-15T14:15:22Z
dc.date.available2020-03-20T18:26:06Z
dc.date.available2022-10-15T14:15:22Z
dc.date.created2020-03-20T18:26:06Z
dc.date.issued2016-05
dc.identifierAceña, Andrés Esteban; Gabach Clement, Maria Eugenia; Extremal black hole initial data deformations; IOP Publishing; Classical and Quantum Gravity; 33; 11; 5-2016; 1-20
dc.identifier0264-9381
dc.identifierhttp://hdl.handle.net/11336/100435
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4395691
dc.description.abstractWe study deformations of axially symmetric initial data for Einstein-Maxwell equations satisfying time-rotation (t-φ) symmetry and containing one asymptotically cylindrical end and one asymptotically flat end. We find that the t-φ symmetry implies the existence of a family of deformed data having the same horizon structure. This result allows us to measure how close the solutions are to the Lichnerowicz equation when arising from nearby free data.
dc.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0264-9381/33/11/115017/meta
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0264-9381/33/11/115017
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectAXIAL SYMMETRY
dc.subjectCYLINDRICAL END
dc.subjectEINSTEIN-MAXWELL EQUATIONS
dc.subjectINITIAL DATA
dc.titleExtremal black hole initial data deformations
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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