Slow roll inflation and BB mode angular power spectrum of CMB
arXiv:1512.03141 · doi:10.1140/epjc/s10052-016-4029-5
Abstract
The BB-mode angular correlation 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.
16 pages, 10 figures
References in corpus (7)
- BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- Inflationary Cosmology
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- Enhanced polarization of CMB from thermal gravitational waves