Sneutrino Tribrid Inflation, Metastable Cosmic Strings and Gravitational Waves
Muhammad Atif Masoud, Mansoor Ur Rehman, Qaisar Shafi

TL;DR
This paper develops a sneutrino-based inflation model within a gauged $U(1)_{B-L}$ extension of the MSSM, linking neutrino masses, leptogenesis, cosmic strings, and gravitational waves, with predictions compatible with current cosmological data.
Contribution
It introduces a novel sneutrino tribrid inflation model that simultaneously explains neutrino masses, reheating, leptogenesis, and predicts metastable cosmic strings and gravitational wave signals.
Findings
Predicted tensor-to-scalar ratio range: $3 imes 10^{-11}$ to $7 imes 10^{-4}$.
B-L breaking scale estimated between $3 imes 10^{14}$ and $2 imes 10^{16}$ GeV.
Cosmic string tension and gravitational wave background compatible with NANOGrav data.
Abstract
We present a successful realization of sneutrino tribrid inflation model based on a gauged extension of Minimal Supersymmetric Standard Model (MSSM). A single interaction term involving the Higgs field and the right-handed neutrinos serves multiple purposes. These include the generation of heavy Majorana masses for the right-handed neutrinos to provide an explanation for the tiny neutrino masses via the seesaw mechanism, a realistic scenario for reheating and non-thermal leptogenesis with a reheat temperature as low as GeV, and a successful realization of inflation with right-handed sneutrino as the inflaton. The matter parity which helps avoid rapid proton decay survives as a subgroup of a -symmetry. Depending on the choice of model parameters yields the following predicted range of the tensor to scalar ratio, $3 \times 10^{-11}\lesssim…
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