Kahler potentials for the MSSM inflation and the spectral index

Abstract

Recently it has been argued that some of the fine-tuning problems of the MSSM inflation associated with the existence of a saddle point along a flat direction may be solved naturally in a class of supergravity models. Here we extend the analysis and show that the constraints on the Kahler potentials in these models are considerably relaxed when the location of the saddle point is treated as a free variable. We also examine the effect of supergravity corrections on inflationary predictions and find that they can slightly alter the value of the spectral index. As an example, for flat direction field values $|{\bar{\varphi }}_0|=1\times 10^{-4}{M}_P$ we find $n\sim \mathrm{0.92...0.94}$ while the prediction of the MSSM inflation without any corrections is $n\sim 0.92$.

13 pages, one figure. Typos corrected and a reference added

References in corpus (3)

• Gauge invariant MSSM inflaton
• Probing the parameter space for an MSSM inflation and the neutralino dark matter
• Graceful exit from a stringy landscape via MSSM inflation

Cited by in corpus (1)

• Kaehler Potentials for Hilltop F-term Hybrid Inflation