BB mode angular power spectrum of CMB from massive gravity
arXiv:1603.05836 · doi:10.1007/s10509-021-04017-2
Abstract
The BB-mode correlation angular power spectrum of CMB is studied for primordial massive gravitational waves for several inflation models. The comparative study of the angular power spectrum with the joint BICEP2/Keck Array and Planck data suggests further constraint on the lower and upper bounds on the mass of primordial gravitons. Assuming a modified dispersion relation, the mass of primordial graviton is also calculated. The resulting constraint also agrees with other theoretical estimates.
11 pages, 7 figures
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