Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2023
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dc.contributor.authorBAGCHI, ARJUNen_US
dc.contributor.authorGrumiller, Danielen_US
dc.contributor.authorSalzer, Jakoben_US
dc.contributor.authorSarkar, Souraven_US
dc.contributor.authorScholler, Friedrichen_US
dc.date.accessioned2019-02-25T09:03:47Z
dc.date.available2019-02-25T09:03:47Z
dc.date.issued2014-10en_US
dc.identifier.citationPhysical Review D, 90(8), 084041.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2023-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.90.084041en_US
dc.description.abstractWe study flat space cosmologies in two dimensions by taking the flat space limit of the AchĂșcarro-Ortiz model. We unravel a phase transition between hot flat space and flat space cosmologies, and derive a new dilaton-dependent counterterm required for the consistency of the Euclidean partition function. Our results generalize to asymptotically mass-dominated two-dimensional dilaton gravity models, whose thermodynamical properties we discuss. The novel case of asymptotic mass domination is covered neither by the comprehensive discussion of Grumiller and McNees [J. High Energy Phys. 04 (2007) 074] nor by the more recent generalization to dilaton gravity with confining U ( 1 ) charges in Grumiller et al. [Phys. Rev. D 90, 044032 (2014)].en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectFlat spaceen_US
dc.subjectCosmologies in two Dimensionsen_US
dc.subjectPhase transitionsen_US
dc.subjectAsymptotic mass dominationen_US
dc.subjectDilaton gravityen_US
dc.subject2014en_US
dc.titleFlat space cosmologies in two dimensions: Phase transitions and asymptotic mass dominationen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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