Kai Schmitz
University of Tokyo
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Featured researches published by Kai Schmitz.
Nuclear Physics | 2012
Wilfried Buchmuller; Valerie Domcke; Kai Schmitz
Abstract The decay of a false vacuum of unbroken B – L symmetry is an intriguing and testable mechanism to generate the initial conditions of the hot early universe. If B – L is broken at the grand unification scale, the false vacuum phase yields hybrid inflation, ending in tachyonic preheating. The dynamics of the B – L breaking Higgs field and thermal processes produce an abundance of heavy neutrinos whose decays generate entropy, baryon asymmetry and gravitino dark matter. We study the phase transition for the full supersymmetric Abelian Higgs model. For the subsequent reheating process we give a detailed time-resolved description of all particle abundances. The competition of cosmic expansion and entropy production leads to an intermediate period of constant ‘reheating’ temperature, during which baryon asymmetry and dark matter are produced. Consistency of hybrid inflation, leptogenesis and gravitino dark matter implies relations between neutrino parameters and superparticle masses. In particular, for a gluino mass of 1 TeV, we find a lower bound on the gravitino mass of 10 GeV.
Journal of High Energy Physics | 2012
Wilfried Buchmuller; Valerie Domcke; Kai Schmitz
A bstractFlavour symmetries of Froggatt-Nielsen type can naturally reconcile the large quark and charged lepton mass hierarchies and the small quark mixing angles with the observed small neutrino mass hierarchies and their large mixing angles. We point out that such a flavour structure, together with the measured neutrino mass squared differences and mixing angles, strongly constrains yet undetermined parameters of the neutrino sector. Treating unknown
Physics Letters B | 2013
Keisuke Harigaya; Masahiro Ibe; Kai Schmitz; Tsutomu T. Yanagida
\mathcal{O}
Physics Letters B | 2014
Keisuke Harigaya; Masahiro Ibe; Kai Schmitz; Tsutomu T. Yanagida
(1) parameters as random variables, we obtain surprisingly accurate predictions for the smallest mixing angle,
Physical Review D | 2013
Keisuke Harigaya; Masahiro Ibe; Kai Schmitz; Tsutomu T. Yanagida
{\text{si}}{{\text{n}}^{{2}}}{2}{\theta_{{{13}}}} = 0.0{7}_{{ - 0.05}}^{{ + 0.11}}
Nuclear Physics | 2011
Wilfried Buchmuller; Kai Schmitz; G. Vertongen
, the smallest neutrino mass,
Physical Review Letters | 2015
Alexander Kusenko; Kai Schmitz; Tsutomu T. Yanagida
{m_{{1}}} = {2}.{2}_{{ - {1}.{4}}}^{{ + 1.7}} \times {1}{0^{{ - {3}}}}{\text{eV}}
Physics Letters B | 2010
Wilfried Buchmuller; Kai Schmitz; G. Vertongen
, and one Majorana phase,
Journal of Cosmology and Astroparticle Physics | 2013
Wilfried Buchmuller; Valerie Domcke; Kai Schmitz
{\alpha_{{{21}}}}/\pi = {1}.0_{{ - 0.2}}^{{ + 0.2}}.
Physics Letters B | 2013
Keisuke Harigaya; Masahiro Ibe; Kai Schmitz; Tsutomu T. Yanagida