Spherical shock waves in general relativity

dc.citation.epage3168en_US
dc.citation.issueNumber10en_US
dc.citation.spage3164en_US
dc.citation.volumeNumber44en_US
dc.contributor.authorNutku, Y.en_US
dc.date.accessioned2016-02-08T10:56:10Z
dc.date.available2016-02-08T10:56:10Z
dc.date.issued1991en_US
dc.departmentDepartment of Mathematicsen_US
dc.description.abstractWe present the metric appropriate to a spherical shock wave in the framework of general relativity. This is a Petrov type-N vacuum solution of the Einstein field equations where the metric is continuous across the shock and the Riemann tensor suffers a step-function discontinuity. Spherical gravitational waves are described by type-N Robinson-Trautman metrics. However, for shock waves the Robinson-Trautman solutions are unacceptable because the metric becomes discontinuous in the Robinson-Trautman coordinate system. Other coordinate systems that have so far been introduced for describing Robinson-Trautman solutions also suffer from the same defect. We shall present the C0-form of the metric appropriate to spherical shock waves using Penrose's approach of identification with warp. Further extensions of Penrose's method yield accelerating, as well as coupled electromagnetic-gravitational shock-wave solutions. © 1991 The American Physical Society.en_US
dc.description.provenanceMade available in DSpace on 2016-02-08T10:56:10Z (GMT). No. of bitstreams: 1 bilkent-research-paper.pdf: 70227 bytes, checksum: 26e812c6f5156f83f0e77b261a471b5a (MD5) Previous issue date: 1991en
dc.identifier.doi10.1103/PhysRevD.44.3164en_US
dc.identifier.issn0556-2821
dc.identifier.urihttp://hdl.handle.net/11693/26183
dc.language.isoEnglishen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.44.3164en_US
dc.source.titlePhysical Review Den_US
dc.titleSpherical shock waves in general relativityen_US
dc.typeArticleen_US

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