pith. machine review for the scientific record. sign in

arxiv: hep-ph/9405337 · v1 · submitted 1994-05-20 · ✦ hep-ph

Recognition: unknown

Flat Potential for Inflaton with a Discrete R-invariance in Supergravity

K. Kumekawa , T. Moroi , T. Yanagida
Authors on Pith no claims yet
classification ✦ hep-ph
keywords inflatondiscreteflatinvariancepotentialsupergravitybaryogenesisbriefly
0
0 comments X
read the original abstract

We show that a very flat potential of inflaton required for a sufficient inflation is naturally obtained in $N=1$ supergravity by imposing a discrete $R$-invariance $Z_{n}$. Several cosmological constraints on parameters in the inflaton superpotential are derived. The reheating temperature turns out to be $(1-10^8)$GeV for the cases of $n$=3--10. Baryogenesis in this model is also discussed briefly.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Nonthermal leptogenesis via cosmological gravitational particle production is tested by inflationary gravitational waves

    hep-ph 2026-05 unverdicted novelty 5.0

    Certain inflation models produce right-handed neutrinos via gravitational effects sufficient for leptogenesis to explain the baryon asymmetry, testable by inflationary gravitational waves.