Inflation in supergravity with a single chiral superfield
From MaRDI portal
Publication:2356376
DOI10.1016/J.PHYSLETB.2014.07.036zbMATH Open1317.83094arXiv1406.0252OpenAlexW2146224415MaRDI QIDQ2356376
Author name not available (Why is that?)
Publication date: 29 July 2015
Published in: (Search for Journal in Brave)
Abstract: We propose new supergravity models describing chaotic Linde- and Starobinsky-like inflation in terms of a single chiral superfield. The key ideas to obtain a positive vacuum energy during large field inflation are (i) stabilization of the real or imaginary partner of the inflaton by modifying a Kahler potential, and (ii) use of the crossing terms in the scalar potential originating from a polynomial superpotential. Our inflationary models are constructed by starting from the minimal Kahler potential with a shift symmetry, and are extended to the no-scale case. Our methods can be applied to more general inflationary models in supergravity with only one chiral superfield.
Full work available at URL: https://arxiv.org/abs/1406.0252
No records found.
This page was built for publication: Inflation in supergravity with a single chiral superfield
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q2356376)