Abstract
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\(\otimes U(1)_{\mathrm{B}\mbox{--}\mathrm{L}}\). In order to obtain a varying neutrino mass, we make an assumption that a soft mass of \(\tilde{Z'}_{\mathrm{BL}}\) 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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Chen, CS., Lin, CM. Bimodal/schizophrenic neutrino as a bridge between inflation and dark energy. Eur. Phys. J. C 71, 1643 (2011). https://doi.org/10.1140/epjc/s10052-011-1643-0
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DOI: https://doi.org/10.1140/epjc/s10052-011-1643-0