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Minimal Supersymmetric Hybrid Inflation, Flipped SU(5) and Proton Decay

Published 24 Dec 2009 in hep-ph and astro-ph.CO | (0912.4737v1)

Abstract: Minimal supersymmetric hybrid inflation utilizes a canonical Kahler potential and a renormalizable superpotential which is uniquely determined by imposing a U(1) R-symmetry. In computing the scalar spectral index $n_s$ we take into account modifications of the tree level potential caused by radiative and supergravity corrections, as well as contributions from the soft supersymmetry breaking terms with a negative soft mass-squared term allowed for the inflaton. All of these contributions play a role in realizing $n_s$ values in the range 0.96-0.97 preferred by WMAP. The U(1) R-symmetry plays an important role in flipped SU(5) by eliminating the troublesome dimension five proton decay. The proton decays into $e+ \pi0$ via dimension six operators arising from the exchange of superheavy gauge bosons with a lifetime of order $10{34}$-$10{36}$ years.

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