Smooth Hybrid Inflation with Low Reheat Temperature and Observable Gravity Waves in SU(5)×U(1)χSU(5) \times U(1)_χ Super-GUT

preprint2022arXivOpen access

Abstract

We realize smooth hybrid inflation in the framework of supersymmetric SU(5)×U(1)χ⊂SO(10)SU(5) \times U(1)_χ\subset SO(10) model which provides a natural solution to the monopole problem appearing in the spontaneous symmetry breaking of SU(5)SU(5). The breaking of U(1)χU(1)_χ symmetry leaves a residual discrete Z2Z_2 symmetry, that serves as the MSSM matter parity, realizing the possibility of the lightest supersymmetric particle as a cold dark matter candidate. The d=5d = 5 proton lifetime for the decay p→K+νˉp \rightarrow K^+ \barν, mediated by color-triplet Higgsinos is found to satisfy current experimental bounds if split-high scale SUSY scenario is employed. We show that with minimal Kähler potential, the soft supersymmetry breaking terms play a vital rôle in bringing the scalar spectral index nsn_s within the Planck's latest bounds. In a minimal Kähler potential setup, small values of tensor-to-scalar ratio r≲3.5×10−7r \lesssim 3.5 \times 10^{-7} are obtained, whereas the gravitino mass turns out to be in the range that favors PeV scale SUSY but is not sufficiently high to avoid the d=5d = 5 proton decay. A non-minimal Kähler potential including higher-order corrections is required to realize successful inflation with central value of scalar spectral index ns=0.9655n_s = 0.9655, large tensor modes r≲0.056r \lesssim 0.056 and a low reheat temperature (3×106≲Tr≲6.5×107)(3\times 10^{6} \lesssim T_r \lesssim 6.5 \times 10^7 ) GeV consistent with leptogenesis and baryogenesis.

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