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On horizons and plane waves

dc.contributor.authorLiu, James T.en_US
dc.contributor.authorZayas, Leopoldo A. Pandoen_US
dc.contributor.authorVaman, Dianaen_US
dc.date.accessioned2006-12-19T19:23:30Z
dc.date.available2006-12-19T19:23:30Z
dc.date.issued2003-10-21en_US
dc.identifier.citationLiu, James T; Zayas, Leopoldo A Pando; Vaman, Diana (2003). "On horizons and plane waves." Classical and Quantum Gravity. 20(20): 4343-4374. <http://hdl.handle.net/2027.42/49210>en_US
dc.identifier.issn0264-9381en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49210
dc.description.abstractWe investigate the possibility of having an event horizon within several classes of metrics that asymptote to the maximally supersymmetric IIB plane wave. We show that the presence of a null Killing vector (not necessarily covariantly constant) implies an effective separation of the Einstein equations into a standard and a wave component. This feature may be used to generate new supergravity solutions asymptotic to the maximally supersymmetric IIB plane wave, starting from standard seed solutions such as branes or intersecting branes in flat space. We find that in many cases it is possible to preserve the extremal horizon of the seed solution. On the other hand, non-extremal deformations of the plane wave solution result in naked singularities. More generally, we prove a no-go theorem against the existence of horizons for backgrounds with a null Killing vector and which contain at most null matter fields. Further attempts at turning on a non-zero Hawking temperature by introducing additional matter have proved unsuccessful. This suggests that one must remove the null Killing vector in order to obtain a horizon. We provide a perturbative argument indicating that this is in fact possible.en_US
dc.format.extent3118 bytes
dc.format.extent347211 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleOn horizons and plane wavesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumMichigan Center for Theoretical Physics, University of Michigan, Ann Arbor, MI 48109-1120, USA; Department of Physics, Princeton University, Princeton, NJ 08544, USAen_US
dc.contributor.affiliationumMichigan Center for Theoretical Physics, University of Michigan, Ann Arbor, MI 48109-1120, USA; School of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540, USAen_US
dc.contributor.affiliationotherDepartment of Physics, Princeton University, Princeton, NJ 08544, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49210/2/q32002.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/0264-9381/20/20/302en_US
dc.identifier.sourceClassical and Quantum Gravity.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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