Majorana CP phases in bi-pair neutrino mixing and leptogenesis
Teruyuki Kitabayashi, Masaki Yasue

TL;DR
This paper estimates Majorana CP phases within bi-pair neutrino mixing, explores their role in leptogenesis, and finds specific phase ranges consistent with observed baryon asymmetry and neutrino mixing angles.
Contribution
It provides a novel analysis of Majorana CP phases in bi-pair neutrino mixing and their implications for leptogenesis within the minimal seesaw model.
Findings
Majorana CP phase is between 0.69 and 0.92 radians.
Phases and are approximately 0.31 to 0.40 radians and -1.25 to -0.32 radians.
The phases satisfy a numerical relation |\u001c|\u2248 2||.
Abstract
We estimate Majorana CP phases for a given flavor neutrino mass matrix (M_\nu) consistent with the bi-pair neutrino mixing, which is recently proposed to describe neutrino mixings given by \sin\theta_{13}=0 for the reactor neutrino mixing, \sin^2\theta_{12} = 1-1/\sqrt{2} for the solar neutrino mixing and either \sin^2\theta_{23} = \tan^2\theta_{12} or \sin^2\theta_{23}=1-\tan^2\theta_{12} for the atmospheric neutrino mixing. Sizes of Majorana CP phases are evaluated so as to generate the observed baryon asymmetry in the universe via a leptogenesis scenario within the framework of the minimal seesaw model, where M_\nu satisfies det(M_\nu)=0 and one active Majorana CP phase (\phi) is present. Assuming the normal mass hierarchy for light neutrinos and one zero texture for a 3X2 Dirac neutrino mass matrix, we find that \phi lies in the region of 0.69<|\phi|<0.92 [rad], which is converted…
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Taxonomy
TopicsNeutrino Physics Research · Particle physics theoretical and experimental studies · Astrophysics and Cosmic Phenomena
