  We develop a model of sneutrino inflation that is charged under $U(1)_{B-L}$
gauge symmetry in no-scale supergravity framework. The model provides an
interesting modification of tribrid inflation. We impose $U(1)_R$ symmetry on
the renormalizable level while allow Planck suppressed non-renormalizable
operators that break R-symmetry. This plays a crucial role in realizing a
Starobinsly-like inflation scenario from one hand. On the other hand it plays
essential role, as well as SUSY breaking effects, in deriving the neutrino
masses from TeV inverse seesaw mechanism. Thus we provide an interpretation for
the extremely small value of the $\mu_S$ mass parameter required for inverse
seesaw mechanism. We discuss the reheating scenario and the possible
constraints on the parameter space in connection to neutrino masses.
