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DC Field | Value | Language |
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dc.contributor.author | BHOWMICK, SUPRITHA | en_US |
dc.contributor.author | GHOSH, DIPTIMOY | en_US |
dc.contributor.author | ULLAH, FARMAN | en_US |
dc.date.accessioned | 2024-10-29T06:44:39Z | |
dc.date.available | 2024-10-29T06:44:39Z | |
dc.date.issued | 2024-10 | en_US |
dc.identifier.citation | Journal of High Energy Physics, 2024(10), 57. | en_US |
dc.identifier.issn | 1029-8479 | en_US |
dc.identifier.uri | https://doi.org/10.1007/JHEP10(2024)057 | en_US |
dc.identifier.uri | http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/9140 | |
dc.description.abstract | In 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.iso | en | en_US |
dc.publisher | Springer Nature | en_US |
dc.subject | Cosmological models | en_US |
dc.subject | de Sitter space | en_US |
dc.subject | 2024 | en_US |
dc.subject | 2024-OCT-WEEK2 | en_US |
dc.subject | TOC-OCT-2024 | en_US |
dc.title | Bispectrum at 1-loop in the Effective Field Theory of Inflation | en_US |
dc.type | Article | en_US |
dc.contributor.department | Dept. of Physics | en_US |
dc.identifier.sourcetitle | Journal of High Energy Physics | en_US |
dc.publication.originofpublisher | Foreign | en_US |
Appears in Collections: | JOURNAL ARTICLES |
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