Reheating constraints on K\"ahler Moduli Inflation
Abstract
The end of inflation is connected to the standard cosmological scenario through reheating. During reheating, the inflaton oscillates around the minimum of the potential and thus decays into the daughter particles that populate the Universe at later times. Using cosmological evolution for observable CMB scales from the time of Hubble crossing to the present time, we translate the constraint on the spectral index from Planck data to the constraint on the reheating scenario in the context of K\"ahler Moduli Inflation. In addition, we extend the de-facto analysis generally done only for the pivot scale to all the observable scales which crossed the Hubble radius during inflation. We study how the maximum number of e-folds varies for different scales, and the effect of the equation of state and potential parameters.
Cite
@article{arxiv.1609.09243,
title = {Reheating constraints on K\"ahler Moduli Inflation},
author = {R. Kabir and A. Mukherjee and D. Lohiya},
journal= {arXiv preprint arXiv:1609.09243},
year = {2016}
}
Comments
10 pages, 6 figures; v(2) submitted to PLB. arXiv admin note: text overlap with arXiv:1502.04673, arXiv:1602.07427 by other authors