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 |