We study the neutrino-photon processes like $\gamma\gamma\to\nu\bar{\nu}$ in the presence of uniform external magnetic field for the case when neutrinos can couple to the electromagnetic field directly through their dipole magnetic moment and obtain the stellar energy loss. The process would be of special relevance in astrophysical situations where standard left-handed neutrinos are trapped and the right handed neutrinos produced through the spin flip interaction induced by neutrino magnetic moment alone can freely stream out
Conserved muonic number may turn out to be a conserved muonic charge, coupled to muonic photons, gam...
The neutrino-nucleon scattering in a collapsing star envelope with a strong magnetic field is invest...
The fermion spin-flip conversion f_L -> f_R + gamma is considered, caused by the difference of the a...
A new type of electromagnetic radiation by a neutrino with non-zero magnetic (and/or electric) momen...
Radiative transition of massless neutrino $\nu_l \to \nu_l + \gamma$ ($l = e, Standard Model. The pr...
The recent studies is reported of the neutrino photoproduction on nuclei, gamma + Ze -> Ze + gamma +...
Motivated by the evidence for a finite neutrino mass we examine anew the interaction of neutrinos in...
After a brief discussion on neutrino electromagnetic properties, we consider the problem of neutrino...
AbstractMotivated by the stringent flux limits for UHE neutrinos coming from gamma ray bursts or act...
The neutrino chirality-flip process under the conditions of the supernova core is investigated in de...
At energies above the threshold for $W$ production the process $\nu \gamma energies. In a cosmologic...
We discuss $\nu - \gamma$ interactions in the presence of a homogeneous magnetic field with energies...
New exact solutions of the modified Dirac equation describing a neutrino with nontrivial electromagn...
AbstractWe examine the effects of magnetic moments of right-handed neutrinos, whose masses are set a...
We study the impact of neutrino magnetic moments on astrophysical neutrinos, in particular supernova...
Conserved muonic number may turn out to be a conserved muonic charge, coupled to muonic photons, gam...
The neutrino-nucleon scattering in a collapsing star envelope with a strong magnetic field is invest...
The fermion spin-flip conversion f_L -> f_R + gamma is considered, caused by the difference of the a...
A new type of electromagnetic radiation by a neutrino with non-zero magnetic (and/or electric) momen...
Radiative transition of massless neutrino $\nu_l \to \nu_l + \gamma$ ($l = e, Standard Model. The pr...
The recent studies is reported of the neutrino photoproduction on nuclei, gamma + Ze -> Ze + gamma +...
Motivated by the evidence for a finite neutrino mass we examine anew the interaction of neutrinos in...
After a brief discussion on neutrino electromagnetic properties, we consider the problem of neutrino...
AbstractMotivated by the stringent flux limits for UHE neutrinos coming from gamma ray bursts or act...
The neutrino chirality-flip process under the conditions of the supernova core is investigated in de...
At energies above the threshold for $W$ production the process $\nu \gamma energies. In a cosmologic...
We discuss $\nu - \gamma$ interactions in the presence of a homogeneous magnetic field with energies...
New exact solutions of the modified Dirac equation describing a neutrino with nontrivial electromagn...
AbstractWe examine the effects of magnetic moments of right-handed neutrinos, whose masses are set a...
We study the impact of neutrino magnetic moments on astrophysical neutrinos, in particular supernova...
Conserved muonic number may turn out to be a conserved muonic charge, coupled to muonic photons, gam...
The neutrino-nucleon scattering in a collapsing star envelope with a strong magnetic field is invest...
The fermion spin-flip conversion f_L -> f_R + gamma is considered, caused by the difference of the a...