Slow-roll inflation and the BB-mode correlation spectrum of the Cosmic Microwave Background

dc.contributor.author Malsawmtluangi, N.
dc.contributor.author Suresh, P. K.
dc.date.accessioned 2022-03-27T11:32:06Z
dc.date.available 2022-03-27T11:32:06Z
dc.date.issued 2017-08-24
dc.description.abstract The BB-mode correlation angular spectrum of cosmic microwave background is studied for several inflation models. A comparative study of the resulting angular power spectrum with the recent joint analysis data of the BICEP2/Keck Array and Planck shows constraint to several slow-roll inflation models of cosmology.
dc.identifier.citation Journal of Physics: Conference Series. v.883(1)
dc.identifier.issn 17426588
dc.identifier.uri 10.1088/1742-6596/883/1/012007
dc.identifier.uri https://iopscience.iop.org/article/10.1088/1742-6596/883/1/012007
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/13866
dc.title Slow-roll inflation and the BB-mode correlation spectrum of the Cosmic Microwave Background
dc.type Conference Proceeding. Conference Paper
dspace.entity.type
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