The parity violating Chern-Simons term in the epoch before the electroweak phase transition can be interpreted as a polarization effect associated to massless right-handed electrons (positrons) in the presence of a large-scale seed hypermagnetic field. We reconfirm the viability of a unified seed field scenario relating the cosmological baryon asymmetry and the origin of the protogalactic large-scale magnetic fields observed in astronomy
We study the evolution of random hypermagnetic fields (HMFs) in the symmetric phase of the early uni...
Within an effective field theory derived from string theory, the universal axion has to be coupled t...
We study the generation of strong magnetic fields in magnetars and in the early universe. For this p...
A tiny hypermagnetic field generated before the electroweak phase transition (EWPT) associated to th...
Primordial cosmological hypermagnetic fields polarize the early Universe plasma prior to the electro...
We study baryon asymmetry generation originated from the leptogenesis in the presence of hypermagnet...
Electroweak baryogenesis proceeds via changes in the non-Abelian Chern-Simons number. It is argued t...
The hypermagnetic helicity density at the electroweak phase transition (EWPT) exceeds many orders of...
We explore the hypothesis that the abundant presence of relativistic antimatter (positrons) in the p...
The generation of the baryon asymmetry of the Universe (BAU) from the hypermagnetic helicity, the ph...
We study the evolution of hypermagnetic fields (HMFs) in random plasma in the symmetric phase of the...
We perform numerical simulations of Cold Electroweak Baryogenesis, including for the first time in t...
At finite hyperconductivity and finite fermionic density the flux lines of long range hypermagnetic ...
AbstractWe study the generation of strong magnetic fields in magnetars and in the early universe. Fo...
We study primordial magnetic field effects on the matter perturbations in the universe. We assume ma...
We study the evolution of random hypermagnetic fields (HMFs) in the symmetric phase of the early uni...
Within an effective field theory derived from string theory, the universal axion has to be coupled t...
We study the generation of strong magnetic fields in magnetars and in the early universe. For this p...
A tiny hypermagnetic field generated before the electroweak phase transition (EWPT) associated to th...
Primordial cosmological hypermagnetic fields polarize the early Universe plasma prior to the electro...
We study baryon asymmetry generation originated from the leptogenesis in the presence of hypermagnet...
Electroweak baryogenesis proceeds via changes in the non-Abelian Chern-Simons number. It is argued t...
The hypermagnetic helicity density at the electroweak phase transition (EWPT) exceeds many orders of...
We explore the hypothesis that the abundant presence of relativistic antimatter (positrons) in the p...
The generation of the baryon asymmetry of the Universe (BAU) from the hypermagnetic helicity, the ph...
We study the evolution of hypermagnetic fields (HMFs) in random plasma in the symmetric phase of the...
We perform numerical simulations of Cold Electroweak Baryogenesis, including for the first time in t...
At finite hyperconductivity and finite fermionic density the flux lines of long range hypermagnetic ...
AbstractWe study the generation of strong magnetic fields in magnetars and in the early universe. Fo...
We study primordial magnetic field effects on the matter perturbations in the universe. We assume ma...
We study the evolution of random hypermagnetic fields (HMFs) in the symmetric phase of the early uni...
Within an effective field theory derived from string theory, the universal axion has to be coupled t...
We study the generation of strong magnetic fields in magnetars and in the early universe. For this p...