Effects of Lightest Neutrino Mass in Leptogenesis

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dc.creatorMolinaro, E.
dc.creatorPetcov, S. T.
dc.creatorShindou, T.
dc.creatorTakanishi, Y.
dc.date2007-09-04
dc.date2008-05-28
dc.date.accessioned2026-07-07T11:42:12Z
dc.date.available2026-07-07T11:42:12Z
dc.descriptionThe effects of the lightest neutrino mass in ``flavoured'' leptogenesis are investigated in the case when the CP-violation necessary for the generation of the baryon asymmetry of the Universe is due exclusively to the Dirac and/or Majorana phases in the neutrino mixing matrix U. The type I see-saw scenario with three heavy right-handed Majorana neutrinos having hierarchical spectrum is considered. The ``orthogonal'' parametrisation of the matrix of neutrino Yukawa couplings, which involves a complex orthogonal matrix R, is employed. Results for light neutrino mass spectrum with normal and inverted ordering (hierarchy) are obtained. It is shown, in particular, that if the matrix R is real and CP-conserving and the lightest neutrino mass m_3 in the case of inverted hierarchical spectrum lies the interval 5 \times 10^{-4} eV < m_3 < 7 \times 10^{-3} eV, the predicted baryon asymmetry can be larger by a factor of \sim 100 than the asymmetry corresponding to negligible m_3 \cong 0. As consequence, we can have successful thermal leptogenesis for 5 \times 10^{-6} eV < m_3 < 5 \times 10^{-2} eV even if R is real and the only source of CP-violation in leptogenesis is the Majorana and/or Dirac phase(s) in U.
dc.description28 pages, 6 figures; published version
dc.identifierhttps://arxiv.org/abs/0709.0413
dc.identifierhttp://arxiv.org/abs/0709.0413
dc.identifierNucl.Phys.B797:93-116,2008
dc.identifierdoi:10.1016/j.nuclphysb.2007.12.033
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200805
dc.subjectHigh Energy Physics - Phenomenology
dc.titleEffects of Lightest Neutrino Mass in Leptogenesis
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