Cosmic Inflation in Minimal $U(1)_{B-L}$ Model: Implications for (Non)
  Thermal Dark Matter and Leptogenesis
  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 $B-L$ extension of the standard model with
three right handed neutrinos. The singlet scalar field responsible for
spontaneous breaking of $B-L$ 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 $Z_2$ 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 non-minimal coupling to
gravity to be at most of order unity. The non-thermal DM scenario is viable,
with or without $Z_2$ symmetry, although in such a case the $B-L$ gauge sector
remains decoupled from the inflationary dynamics due to tiny couplings. We also
show that the reheat temperature predicted by the model prefers non-thermal
leptogenesis with hierarchical right handed neutrinos while being consistent
with other requirements.
