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Reheat temperature in supersymmetric hybrid inflation models

2004/12/31 by V. N. Senoguz, Q. Shafi · 1 citation
Physics and Astronomy · #hep-ph

paper · pdf · doi:10.1103/physrevd.71.043514

published as Phys.Rev.D71:043514,2005 · 15 pages, 8 figures, revtex4. v2: minor changes, matches published version

arxiv created 2005/02/25 · arxiv updated 2009/12/01

Abstract

The allowed range of parameters for supersymmetric hybrid inflation and its extensions are investigated. The lower bound on the reheat temperature Tr in these models with hierarchical right handed neutrinos is found to be 3*107 GeV. (Tr as low as 100 GeV is possible for quasi degenerate right handed neutrinos.) We also present revised estimates for the scalar spectral index and the symmetry breaking scale associated with inflation.

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