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Non-Extremal Gravity Duals for Fractional D3-Branes on the Conifold

dc.contributor.authorBuchel, Alexanderen_US
dc.contributor.authorKlebanov, Igor R.en_US
dc.contributor.authorHerzog, Christopher P.en_US
dc.contributor.authorZayas, Leopoldo A. Pandoen_US
dc.contributor.authorTseytlin, Arkady A.en_US
dc.date.accessioned2006-12-19T19:15:47Z
dc.date.available2006-12-19T19:15:47Z
dc.date.issued2001-04-01en_US
dc.identifier.citationBuchel, Alexander; Klebanov, Igor R.; Herzog, Christopher P.; Zayas, Leopoldo Pando; Tseytlin, Arkady A. (2001). "Non-Extremal Gravity Duals for Fractional D3-Branes on the Conifold." Journal of High Energy Physics. 04(033). <http://hdl.handle.net/2027.42/49115>en_US
dc.identifier.issn1126-6708en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49115
dc.description.abstractThe world volume theory on N regular and M fractional D3-branes at the conifold singularity is a non-conformal N = 1 supersymmetric SU (N+M) × SU(N) gauge theory. In previous work the extremal Type IIB supergravity dual of this theory at zero temperature was constructed. Regularity of the solution requires a deformation of the conifold: this is a reflection of the chiral symmetry breaking. To study the non-zero temperature generalizations non-extremal solutions have to be considered, and in the high temperature phase the chiral symmetry is expected to be restored. Such a solution is expected to have a regular Schwarzschild horizon. We construct an ansatz necessary to study such non-extremal solutions and show that the simplest possible solution has a singular horizon. We derive the system of second order equations in the radial variable whose solutions may have regular horizons.en_US
dc.format.extent3118 bytes
dc.format.extent339935 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleNon-Extremal Gravity Duals for Fractional D3-Branes on the Conifolden_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumMichigan Center for Theoretical Physics, The University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherInstitute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030, USAen_US
dc.contributor.affiliationotherInstitute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030, USA; Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08544, USAen_US
dc.contributor.affiliationotherJoseph Henry Laboratories, Princeton University, Princeton, New Jersey 08544, USAen_US
dc.contributor.affiliationotherDepartment of Physics, The Ohio State University, Columbus, OH 43210, USA; Blackett Laboratory, Imperial College, London SW7 2BZ, U.K.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49115/2/jhep042001033.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/1126-6708/2001/04/033en_US
dc.identifier.sourceJournal of High Energy Physics.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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