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$\otimes U(1)_{ B-L}$. In order to obtain a varying neutrino mass, we make an assumption that a soft mass of $\tilde{ Z'}_{ BL}$ 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.
Categories: hep-ph astro-ph.CO