We have studied the two-body production and decay of a heavy, right-handed neutrino to two light states using the full Boltzmann equation instead of the usual integrated Boltzmann equation which assumes kinetic equilibrium of all species. Decays and inverse decays are inefficient for thermalising the distribution function of the heavy neutrino and in some parameter ranges there can be very large deviations from kinetic equilibrium. This leads to substantial numerical differences between the two approaches. Furthermore we study the impact of this difference on the lepton asymmetry production during leptogenesis and find that in the strong washout regime the final asymmetry is changed by 15-30% when the full Boltzmann equation is used
AbstractWe briefly review the main aspects of leptogenesis, pointing out the main reasons that draw ...
The mass term for Majorana neutrinos explicitly violates lepton number. Several authors have used th...
Neutrino oscillations, the evidence of dark matter and the baryon asymmetry in the universe can not ...
We consider the full Boltzmann equations for standard and soft leptogenesis, instead of the usual in...
We work out the thermodynamic equations for the decays and scatterings of heavy Majorana neutrinos i...
In many phenomenologically interesting models of thermal leptogenesis the heavy neutrinos are non-re...
We propose a new mechanism producing a non-vanishing lepton number asymmetry, based on decays of hea...
We study the evolution of a cosmological baryon asymmetry produced via leptogenesis by means of the ...
Spectator processes which are in thermal equilibrium during the period of baryogenesis influence the...
Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origi...
We discuss leptogenesis in a model with heavy right-handed Majorana neutrinos propagating in a const...
During the process of thermal leptogenesis temperature decreases by about one order of magnitude whi...
Leptogenesis can successfully explain the matter-antimatter asymmetry via out-of-equilibrium decays ...
We study a class of leptogenesis models where the light neutrinos acquire their observed small masse...
Wörmann M. Aspects of nonequilibrium in Leptogenesis. Bielefeld: Universität Bielefeld; 2016
AbstractWe briefly review the main aspects of leptogenesis, pointing out the main reasons that draw ...
The mass term for Majorana neutrinos explicitly violates lepton number. Several authors have used th...
Neutrino oscillations, the evidence of dark matter and the baryon asymmetry in the universe can not ...
We consider the full Boltzmann equations for standard and soft leptogenesis, instead of the usual in...
We work out the thermodynamic equations for the decays and scatterings of heavy Majorana neutrinos i...
In many phenomenologically interesting models of thermal leptogenesis the heavy neutrinos are non-re...
We propose a new mechanism producing a non-vanishing lepton number asymmetry, based on decays of hea...
We study the evolution of a cosmological baryon asymmetry produced via leptogenesis by means of the ...
Spectator processes which are in thermal equilibrium during the period of baryogenesis influence the...
Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origi...
We discuss leptogenesis in a model with heavy right-handed Majorana neutrinos propagating in a const...
During the process of thermal leptogenesis temperature decreases by about one order of magnitude whi...
Leptogenesis can successfully explain the matter-antimatter asymmetry via out-of-equilibrium decays ...
We study a class of leptogenesis models where the light neutrinos acquire their observed small masse...
Wörmann M. Aspects of nonequilibrium in Leptogenesis. Bielefeld: Universität Bielefeld; 2016
AbstractWe briefly review the main aspects of leptogenesis, pointing out the main reasons that draw ...
The mass term for Majorana neutrinos explicitly violates lepton number. Several authors have used th...
Neutrino oscillations, the evidence of dark matter and the baryon asymmetry in the universe can not ...