2010/11/30 by Renata Kallosh, Andrei Linde, Tomas Rube · 1 citation
Physics and Astronomy · #hep-th #astro-ph.HE #gr-qc #hep-ph
paper · pdf · doi:10.1103/physrevd.83.043507
published as Phys.Rev.D83:043507,2011 · 6 pages
arxiv created 2010/12/10 · arxiv updated 2011/02/18
We describe a way to construct supergravity models with an arbitrary inflaton potential V (ϕ) and show that all other scalar fields in this class of models can be stabilized at the inflationary trajectory by a proper choice of the Kähler potential.