Chaotic inflation and baryogenesis by right-handed sneutrinos

We present a model of chaotic inflation driven by the superpartner of the right-handed neutrino (Ñ \~R). This model gives the correct magnitude of the density perturbation observed by the Cosmic Background Explorer satellite with a right-handed neutrino mass {}10¹³ GeV, which is also preferred by the Mikheyev-Smirnov-Wolfenstein solution to the solar neutrino problem. The reheating process is the dacay of the coherently oscillating Ñ \~R. This decay process also generates lepton asymmetry via CP violation, which will be converted to baryon asymmetry thanks to the electroweak anomaly. This model can incorporate the {τ}-neutrino mass {}10 eV.