Inflation, Gravitino and Reheating in Modified Modular invariant Supergravity
Mitsuo J. Hayashi, Yuta Koshimizu, Toyokazu Fukuoka, Kenji Takagi and, Hikoya Kasari

TL;DR
This paper proposes a modified string-inspired supergravity model that successfully explains inflation, matches WMAP observations, and predicts observable signatures for future experiments, linking particle physics and cosmology.
Contribution
It introduces a new modular invariant supergravity model that addresses key inflationary issues and provides concrete predictions for cosmological parameters and particle production.
Findings
Model clears the η-problem and negative energy issues.
Predicted scalar spectral index n_s ≈ 0.9746.
Reheating temperature estimated at 3.88×10^7 GeV.
Abstract
A new modified string-inspired modular invariant supergravity model is proposed and is applied to realize the slow roll inflation in Einstein frame. Because inflation deals with Planck scale physics, the dilaton can be a strong candidate for identification with the inflaton. The model we used, cleared the -problem and negative energy problem of potential at stable point, and appeared to predict successfully the values of observations at the inflation era. We proved that the model explains WMAP observations appropriately. Moreover, a mechanism of SSB and Gravitino production just after the end of inflation is investigated. We have obtained power spectrum of the density perturbation as and the scalar spectral index as and its tilt as . The ratio between scalar power spectrum and…
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