Slow-roll inflation and BB-mode angular power spectrum of CMB

dc.contributor.author Malsawmtluangi, N.
dc.contributor.author Suresh, P. K.
dc.date.accessioned 2022-03-27T11:32:07Z
dc.date.available 2022-03-27T11:32:07Z
dc.date.issued 2016-05-01
dc.description.abstract The BB-mode correlation angular power spectrum of CMB is obtained by considering the primordial gravitational waves in the squeezed vacuum state for various inflationary models and results are compared with the joint analysis of the BICEP2/Keck Array and Planck 353 GHz data. The present results may constrain several models of inflation.
dc.identifier.citation European Physical Journal C. v.76(5)
dc.identifier.issn 14346044
dc.identifier.uri 10.1140/epjc/s10052-016-4029-5
dc.identifier.uri http://link.springer.com/10.1140/epjc/s10052-016-4029-5
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/13867
dc.title Slow-roll inflation and BB-mode angular power spectrum of CMB
dc.type Journal. Article
dspace.entity.type
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