A CFT interpretation of cosmological correlation functions in α−vacua in de-Sitter space

dc.contributor.authorJAIN, SACHINen_US
dc.contributor.authorKundu, Nilayen_US
dc.contributor.authorKundu, Sumanen_US
dc.contributor.authorMEHTA, ABHISHEKen_US
dc.contributor.authorSake, Sunil Kumaren_US
dc.contributor.departmentDept. of Physicsen_US
dc.date.accessioned2023-06-26T03:56:27Z
dc.date.available2023-06-26T03:56:27Z
dc.date.issued2023-05en_US
dc.description.abstractDe-Sitter(dS) space allows for a generalized class of vacua, known as α–vacua, described by some parameters. The Bunch-Davies (BD) vacuum is a point in this parameter space. The cosmological correlation function in BD vacuum in four dimensions and can be interpreted as CFT3 correlation function of certain operators. However, the correlation function in α–vacua takes a much more complicated form. In this paper, we give a simple prescription to compute correlation function in α–vacua in terms of correlation function of BD vacuum. We also show that the correlation function in the α–vacua can be related to three-dimensional CFT correlation functions if we relax the requirement of consistency with OPE limit. Relaxation of consistency with OPE limit can be naturally achieved in momentum space.en_US
dc.identifier.citationJournal of High Energy Physics, 2023(05), 111.en_US
dc.identifier.issn1029-8479en_US
dc.identifier.sourcetitleJournal of High Energy Physicsen_US
dc.identifier.urihttps://doi.org/10.1007/JHEP05(2023)111
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/8045
dc.language.isoenen_US
dc.publication.originofpublisherForeignen_US
dc.publisherSpringer Natureen_US
dc.subjectConformal and W Symmetryen_US
dc.subjectScale and Conformal Symmetriesen_US
dc.subjectSpace-Time Symmetriesen_US
dc.subject2023-JUN-WEEK1en_US
dc.subjectTOC-JUN-2023en_US
dc.subject2023en_US
dc.titleA CFT interpretation of cosmological correlation functions in α−vacua in de-Sitter spaceen_US
dc.typeArticleen_US

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