Publication:
Completely regular quantum stress tensor with w < -1

dc.contributor.coauthorKahya, Ercan O.
dc.contributor.coauthorWoodard, R. P.
dc.contributor.departmentDepartment of Physics
dc.contributor.departmentDepartment of Physics
dc.contributor.kuauthorÖnemli, Vakıf Kemal
dc.contributor.schoolcollegeinstituteCollege of Sciences
dc.date.accessioned2024-11-09T12:25:01Z
dc.date.issued2010
dc.description.abstractFor many quantum field theory computations in cosmology it is not possible to use the flat space trick of obtaining full, interacting states by evolving free states over infinite times. State wave functionals must be specified at finite times and, although the free states suffice to obtain the lowest order effects, higher order corrections necessarily involve changes of the initial state. Failing to correctly change the initial state can result in effective field equations which diverge on the initial value surface, or which contain tedious sums of terms that redshift like inverse powers of the scale factor. In this paper we verify a conjecture from 2004 that the lowest order initial state correction can indeed absorb the initial value divergences and all the redshifting terms of the two-loop expectation value (in free, Bunch-Davies vacuum) of the stress tensor of a massless, minimally coupled scalar with a quartic self-interaction on a nondynamical de Sitter background.
dc.description.fulltextYES
dc.description.indexedbyWoS
dc.description.indexedbyScopus
dc.description.issue2
dc.description.openaccessYES
dc.description.publisherscopeInternational
dc.description.sponsoredbyTubitakEuTÜBİTAK
dc.description.sponsorshipScientific and Technological Research Council of Turkey (TÜBİTAK)
dc.description.sponsorshipNSF
dc.description.sponsorshipInstitute for Fundamental Theory at the University of Florida
dc.description.versionPublisher version
dc.description.volume81
dc.formatpdf
dc.identifier.doi10.1103/PhysRevD.81.023508
dc.identifier.eissn2470-0029
dc.identifier.embargoNO
dc.identifier.filenameinventorynoIR00768
dc.identifier.issn2470-0010
dc.identifier.linkhttps://doi.org/10.1103/PhysRevD.81.023508
dc.identifier.quartileN/A
dc.identifier.scopus2-s2.0-77649200597
dc.identifier.urihttps://hdl.handle.net/20.500.14288/1525
dc.identifier.wos275068900024
dc.keywordsGeneralized chaplygin-gas
dc.keywordsNull energy condition
dc.keywordsExpectation value formalism
dc.keywordsCoupled scalar field
dc.keywordsDark energy
dc.keywordsQuintom model
dc.keywordsSitter space
dc.keywordsCosmological models
dc.keywordsVacuum polarization
dc.keywordsModified gravity
dc.languageEnglish
dc.publisherAmerican Physical Society (APS)
dc.relation.grantno108T009 - 107T896 - BIDEB 2221
dc.relation.grantnoPHY-0653085
dc.relation.urihttp://cdm21054.contentdm.oclc.org/cdm/ref/collection/IR/id/765
dc.sourcePhysical Review D
dc.subjectPhysics
dc.subjectAstronomy and astrophysics
dc.titleCompletely regular quantum stress tensor with w < -1
dc.typeJournal Article
dspace.entity.typePublication
local.contributor.kuauthorÖnemli, Vakıf Kemal
relation.isOrgUnitOfPublicationc43d21f0-ae67-4f18-a338-bcaedd4b72a4
relation.isOrgUnitOfPublication.latestForDiscoveryc43d21f0-ae67-4f18-a338-bcaedd4b72a4

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