Null singularity formation by scalar fields in colliding waves and black holes

dc.authorid0000-0001-9344-5786en_US
dc.authorid0000-0003-1980-4829en_US
dc.contributor.authorGürtuğ, Özay
dc.contributor.authorHalilsoy, Mustafa
dc.contributor.authorGürtuğ, Özay
dc.date.accessioned2024-07-12T20:59:05Z
dc.date.available2024-07-12T20:59:05Z
dc.date.issued2002en_US
dc.departmentFakülteler, Mühendislik ve Doğa Bilimleri Fakültesi, Yazılım Mühendisliği Bölümüen_US
dc.description.abstractIt was believed that when gravitational, electromagnetic and scalar waves interact, a spacelike curvature singularity or Cauchy horizon develops because of mutual focusing. We show with an exact solution that the collision of Einstein-Maxwell-Scalar fields, in contrast to previous studies, predicts singularities on null surfaces and that this is a transition phase between spacelike singularities and regular horizons. Divergences of tidal forces in the null singularities is shown to be weaker relative to the spacelike ones. Using the local isometry between colliding plane waves and black holes, we show that the inner horizon of Reissner-Nordstrom black hole transforms into a null singularity when a particular scalar field is coupled to it. We also present an analytic exact solution, which represents a Reissner-Nordstrom black hole with scalar hair in between the ergosphere.en_US
dc.identifier.citationGürtuğ, Ö. ve Halilsoy, M. (2002). Null singularity formation by scalar fields in colliding waves and black holes. Arxiv. s. 1-23.en_US
dc.identifier.endpage23en_US
dc.identifier.startpage1en_US
dc.identifier.urihttps://arxiv.org/abs/gr-qc/0203019
dc.identifier.urihttps://hdl.handle.net/20.500.12415/3263
dc.language.isoenen_US
dc.publisherCornell Universityen_US
dc.relation.ispartofArxiven_US
dc.relation.publicationcategoryDiğeren_US
dc.rightsAttribution-NonCommercial 3.0 United States*
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc/3.0/us/*
dc.snmzKY00345
dc.titleNull singularity formation by scalar fields in colliding waves and black holesen_US
dc.typeArticle
dspace.entity.typePublication

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