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. 
John Ellis, Marcos A. G. Garcia, Natsumi Nagata, Dimitri V.   Nanopoulos, Keith A. Olive
hep-ph astro-ph.CO gr-qc hep-th