Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/9140
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dc.contributor.authorBHOWMICK, SUPRITHAen_US
dc.contributor.authorGHOSH, DIPTIMOYen_US
dc.contributor.authorULLAH, FARMANen_US
dc.date.accessioned2024-10-29T06:44:39Z
dc.date.available2024-10-29T06:44:39Z
dc.date.issued2024-10en_US
dc.identifier.citationJournal of High Energy Physics, 2024(10), 57.en_US
dc.identifier.issn1029-8479en_US
dc.identifier.urihttps://doi.org/10.1007/JHEP10(2024)057en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/9140
dc.description.abstractIn this paper we compute 1-loop corrections to the bispectrum in the decoupling limit of the Effective Field Theory of Inflation (EFToI). We regulate the divergences by employing dimensional regularization and work in d = 3 + δ dimensions. We find that the final results feature analytic structures of the form log (ki/kT) and log (H/μ), where H is the Hubble parameter and μ is the renormalisation scale. An interesting outcome of our calculations is that unlike the 1-loop correction to the power-spectrum computed in [1] the unrenormalised answers always produce unphysical logarithms of co-moving momenta. These unphysical logarithms are cancelled only after renormalisation. We expect this to be a generic feature for loop computations unless there is some cancellation as in the previously computed 1-loop result for the power-spectrum.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectCosmological modelsen_US
dc.subjectde Sitter spaceen_US
dc.subject2024en_US
dc.subject2024-OCT-WEEK2en_US
dc.subjectTOC-OCT-2024en_US
dc.titleBispectrum at 1-loop in the Effective Field Theory of Inflationen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleJournal of High Energy Physicsen_US
dc.publication.originofpublisherForeignen_US
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