Leptogenesis and Neutrino Masses in an Inflationary SUSY Pati-Salam Model
C. Pallis, N. Toumbas

TL;DR
This paper presents a SUSY Pati-Salam inflationary model that successfully explains non-thermal leptogenesis, neutrino masses, and baryon asymmetry, consistent with current observational data and avoiding monopole overproduction.
Contribution
It introduces a novel inflationary scenario within SUSY Pati-Salam GUT that incorporates non-thermal leptogenesis with specific neutrino mass predictions and observational consistency.
Findings
Inflation driven by a quartic Higgs potential with non-minimal gravity coupling.
Reproduction of observed baryon asymmetry through right-handed neutrino decay.
Constraints on neutrino masses and right-handed neutrino scales consistent with data.
Abstract
We implement the mechanism of non-thermal leptogenesis in the framework of an inflationary model based on a supersymmetric (SUSY) Pati-Salam Grand Unified Theory (GUT). In particular, we show that inflation is driven by a quartic potential associated with the Higgs fields involved in the spontaneous GUT symmetry breaking, in the presence of a non-minimal coupling of the inflaton field to gravity. The inflationary model relies on renormalizable superpotential terms and does not lead to overproduction of magnetic monopoles. It is largely independent of one-loop radiative corrections, and it can be consistent with current observational data on the inflationary observables, with the GUT symmetry breaking scale assuming its SUSY value. Non-thermal leptogenesis is realized by the out-of-equilibrium decay of the two lightest right-handed (RH) neutrinos, which are produced by the inflaton…
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