Bimodal/Schizophrenic Neutrino As a Bridge between Inflation and Dark Energy

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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10 pages; accepted for publication in Eur. Phys. J. C

Scientific paper

10.1140/epjc/s10052-011-1643-0

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.

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