We investigate the effect of the presence of non-pure fermionic neutrinos on the relativistic effective degrees of freedom in the early universe. The statistics of neutrinos is transformed continuously from Fermi-Dirac to Maxwell-Boltzmann statistics. We find that the relativistic degrees of freedom decreases with the deviation from pure Fermi-Dirac statistics of neutrinos if there are constant and large lepton asymmetries. Additionally, we confirm that the change of the statistics of neutrinos from Fermi-Dirac to Maxwell-Boltzmann is not sufficient to cover the excess of the effective number of neutrinos.
We study effects of CP violation in a modified bipair neutrino mixing scheme
predicting $\sin^2\theta_{23}$ near both 0.4 and 0.6 currently consistent with
experimentally allowed values. The source of CP violation is supplied by
charged lepton mixing accompanied by a single phase, whose mixing size is
assumed to be less than that of the Wolfenstein parameter for the quark mixing.
Including results of leptogenesis, which is based on the minimal seesaw model,
we obtain the allowed region of CP-violating Dirac and Majorana phases, which
provides the observed baryon asymmetry of the universe in the case of the Dirac
neutrino mass matrix subject to one zero texture.Comment: 5 pages, 30 figures, accepted for publication in Physics Letters
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