Cosmic Inflation in Minimal $U(1)_{B-L}$ Model: Implications for (Non) Thermal Dark Matter and Leptogenesis
Debasish Borah, Suruj Jyoti Das, Abhijit Kumar Saha

TL;DR
This paper explores a minimal $U(1)_{B-L}$ model where the singlet scalar acts as the inflaton, analyzing implications for dark matter, baryon asymmetry, and neutrino masses, highlighting challenges with thermal dark matter overproduction.
Contribution
It provides a detailed RGE analysis of inflationary dynamics in a minimal $B-L$ model, demonstrating the viability of non-thermal dark matter and leptogenesis scenarios.
Findings
Thermal dark matter is overproduced due to limited annihilation channels.
Non-thermal dark matter remains viable with decoupled $B-L$ sector.
Reheat temperature favors non-thermal leptogenesis with hierarchical neutrinos.
Abstract
We study the possibility of realising cosmic inflation, dark matter (DM), baryon asymmetry of the universe (BAU) and light neutrino masses in non-supersymmetric minimal gauged extension of the standard model with three right handed neutrinos. The singlet scalar field responsible for spontaneous breaking of gauge symmetry also plays the role of inflaton by virtue of its non-minimal coupling to gravity. While the lightest right handed neutrino is the DM candidate, being stabilised by an additional symmetry, we show by performing a detailed renormalisation group evolution (RGE) improved study of inflationary dynamics that thermal DM is generally overproduced due to insufficient annihilations through gauge and scalar portals. This happens due to strict upper limits obtained on gauge and other dimensionless couplings responsible for DM annihilation while assuming the…
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