In unified theories with right-handed neutrinos the scale of B − L breaking can a priori vary between the unification scale and the Fermi scale of electroweak symmetry breaking. We derive upper and lower bounds on the masses of light and heavy Majorana neutrinos and on the scale of B − L breaking from the requirement that the cosmological baryon asymmetry is generated before the electroweak phase transition. Baryogenesis poses a serious problem for extended gauge theories with heavy neutrinos and neutral vector bosons in the TeV mass range
We show that certain models for neutrino masses that lead to the MSW explanation of the solar neutri...
Due to sphaleron processes in the high-temperature symmetric phase of the standard model the cosmolo...
We study the effect on leptogenesis due to B-L cosmic strings of a U(1)(B-L) extension of the Standa...
In the standard model and most of its extensions the electroweak transition is too weak to affect th...
Baryogenesis via leptogenesis is an attractive scenario that links the physics of right handed neutr...
The current status of baryogenesis is reviewed, with an emphasis on electroweak baryogenesis and lep...
We study the scale at which one can generate the lepton asymmetry of the universe which could then g...
It is shown that the requirement of preservation of baryon asymmetry does not rule out a scale for l...
In theories where B - L is a spontaneously broken local symmetry, the cosmological baryon asymmetry ...
We study the implications of neutral heavy gauge bosons to electroweak (EW) baryogenesis, neutrino p...
Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origi...
We study the simplest theories with exact spacetime parity that solve the strong CP problem and succ...
If the neutrino is Majorana type and the electroweak phase transition is second or weak first order,...
If the neutrino is Majorana type and the electroweak phase transition is second or weak first order,...
We study the implications of neutral heavy gauge bosons to electroweak (EW) baryogenesis, neutrino p...
We show that certain models for neutrino masses that lead to the MSW explanation of the solar neutri...
Due to sphaleron processes in the high-temperature symmetric phase of the standard model the cosmolo...
We study the effect on leptogenesis due to B-L cosmic strings of a U(1)(B-L) extension of the Standa...
In the standard model and most of its extensions the electroweak transition is too weak to affect th...
Baryogenesis via leptogenesis is an attractive scenario that links the physics of right handed neutr...
The current status of baryogenesis is reviewed, with an emphasis on electroweak baryogenesis and lep...
We study the scale at which one can generate the lepton asymmetry of the universe which could then g...
It is shown that the requirement of preservation of baryon asymmetry does not rule out a scale for l...
In theories where B - L is a spontaneously broken local symmetry, the cosmological baryon asymmetry ...
We study the implications of neutral heavy gauge bosons to electroweak (EW) baryogenesis, neutrino p...
Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origi...
We study the simplest theories with exact spacetime parity that solve the strong CP problem and succ...
If the neutrino is Majorana type and the electroweak phase transition is second or weak first order,...
If the neutrino is Majorana type and the electroweak phase transition is second or weak first order,...
We study the implications of neutral heavy gauge bosons to electroweak (EW) baryogenesis, neutrino p...
We show that certain models for neutrino masses that lead to the MSW explanation of the solar neutri...
Due to sphaleron processes in the high-temperature symmetric phase of the standard model the cosmolo...
We study the effect on leptogenesis due to B-L cosmic strings of a U(1)(B-L) extension of the Standa...