Starobinsky-Like Inflation and Neutrino Masses in a No-Scale SO(10)
  Model
  Using a no-scale supergravity framework, we construct an SO(10) model that
makes predictions for cosmic microwave background observables similar to those
of the Starobinsky model of inflation, and incorporates a double-seesaw model
for neutrino masses consistent with oscillation experiments and late-time
cosmology. We pay particular attention to the behaviour of the scalar fields
during inflation and the subsequent reheating.
