Add to ORKGElectroweak baryogenesis could be very efficient at the end of an electroweak-scale inflation. Reheating that followed inflation could create a highly non-equilibrium plasma, in which the baryon number violating transitions were rapid. In addition, the time-dependent motions of the scalar degrees of freedom could provide the requisite CP violation. If the final reheat temperature was below 100 GeV, there was no wash-out of the baryon asymmetry after thermalization. The observed value of the baryon asymmetry can be attained in a number of models, some of which do not require a significant departure from the Standard Model
We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson whose inter...
In this work we show that the new bounds on the Higgs mass are more than difficult to reconcile with...
AbstractWe show that a baryon asymmetry can be generated by dissipative effects during warm inflatio...
We propose a new alternative for baryogenesis which resolves a number of the problems associated wit...
The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium condition...
It has recently been suggested that the baryon washout problem of the standard electroweak baryogene...
The usual sphaleron bound and the statement of the impossibility of baryon production at a second or...
The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium condition...
Thermal inflation can solve serious cosmological problems such as overproduction of gravitinos and m...
Cold electroweak baryogenesis was proposed as a scenario to bypass generic problems of electroweak b...
We explore viable scenarios for parametric resonant amplification of electroweak (EW) gauge fields a...
The realisation that the electroweak anomaly can induce significant baryon number violation at high ...
At the end of inflation the universe is frozen in a near zero-entropy state with energy density in a...
The thermal average of the Polyakov line is non-zero at high temperature. It has been suggested that...
Baryogenesis at the end of extended inflation is studied. Extended inflation is brought to an end by...
We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson whose inter...
In this work we show that the new bounds on the Higgs mass are more than difficult to reconcile with...
AbstractWe show that a baryon asymmetry can be generated by dissipative effects during warm inflatio...
We propose a new alternative for baryogenesis which resolves a number of the problems associated wit...
The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium condition...
It has recently been suggested that the baryon washout problem of the standard electroweak baryogene...
The usual sphaleron bound and the statement of the impossibility of baryon production at a second or...
The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium condition...
Thermal inflation can solve serious cosmological problems such as overproduction of gravitinos and m...
Cold electroweak baryogenesis was proposed as a scenario to bypass generic problems of electroweak b...
We explore viable scenarios for parametric resonant amplification of electroweak (EW) gauge fields a...
The realisation that the electroweak anomaly can induce significant baryon number violation at high ...
At the end of inflation the universe is frozen in a near zero-entropy state with energy density in a...
The thermal average of the Polyakov line is non-zero at high temperature. It has been suggested that...
Baryogenesis at the end of extended inflation is studied. Extended inflation is brought to an end by...
We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson whose inter...
In this work we show that the new bounds on the Higgs mass are more than difficult to reconcile with...
AbstractWe show that a baryon asymmetry can be generated by dissipative effects during warm inflatio...