We consider the possibility to combine inflection point inflation and growing neutrino dark energy in a particular setup of bimodal/schizophrenic neutrino model in the framework of MSSM ⊗U(1)B--L⊗U(1)B--L . In order to obtain a varying neutrino mass, we make an assumption that a soft mass of Z′~BLZ′~BL depends on a scalar field which plays the role of a cosmon field. We also investigate the possible effects of the cosmon field in the early universe such as modulated reheating and found that the induced density perturbation is negligible.
Relation:
The European Physical Journal C 71(5), 1643(article id.)
