Using the density matrix equations (DME) for high scale leptogenesis based on the type I seesaw mechanism, in which the CP violation (CPV) is provided by the low-energy Dirac or/and Majorana phases of the neutrino mixing (PMNS) matrix, we investigate the 1-to-2 and the 2-to-3 flavour regime transitions, where the 1, 2 and 3 leptogenesis flavour regimes in the generation of the baryon asymmetry of the Universe (BAU) are described by the Boltzmann equations. Concentrating on the 1-to-2 flavour transition we determine the general conditions under which the BAU goes through zero and changes sign in the transition. Analysing in detail the behaviour of the BAU in the transition in the case of two heavy Majorana neutrinos with hierarchical masses ...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
The CP-violation necessary for the generation of the baryon asymmetry of the Universe YB in the "fla...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...
The biunitary parametrization of the neutrino Dirac mass matrix m(D) of the seesaw mechanism of neut...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
Abstract We revisit the possibility of producing the observed baryon asymmetry of the Universe via t...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
The effects of the lightest neutrino mass in "flavoured" leptogenesis are investigated in the case w...
The biunitary parametrization of the neutrino Dirac mass matrix mD of the seesaw mechanism of neutri...
Taking into account the recent progress in the understanding of the lepton flavour effects in lep...
Flavour effects due to lepton interactions in the early Universe may have played an important role i...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
The CP-violation necessary for the generation of the baryon asymmetry of the Universe YB in the "fla...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...
The biunitary parametrization of the neutrino Dirac mass matrix m(D) of the seesaw mechanism of neut...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
Abstract We revisit the possibility of producing the observed baryon asymmetry of the Universe via t...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
The effects of the lightest neutrino mass in "flavoured" leptogenesis are investigated in the case w...
The biunitary parametrization of the neutrino Dirac mass matrix mD of the seesaw mechanism of neutri...
Taking into account the recent progress in the understanding of the lepton flavour effects in lep...
Flavour effects due to lepton interactions in the early Universe may have played an important role i...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...
We revisit the possibility of producing the observed baryon asymmetry of the Universe via thermal le...
The CP-violation necessary for the generation of the baryon asymmetry of the Universe YB in the "fla...
We consider leptogenesis in a left-right-symmetric seesaw scenario in which neutrino mass generation...