activity
19942021
most citedInstability of magnetic fields in electroweak plasma driven by neutrino asymmetries

54 citations · 717 across the 52 of their papers we have counts for

collaborators
Showing 1998 · hep-phShow all

7 papers · 2 filters

hep-ph1998★ 21 cited

Neutrino Conversions in Solar Random Magnetic Fields

V. B Semikoz, E. Torrente-Lujan

We consider the effect of a random magnetic field in the convective zone of the Sun superimposed to a regular magnetic field on resonant neutrino spin-flavour oscillations. We argu…

hep-ph1998★ 1 cited

Neutrino electron scattering and electroweak gauge structure: Probing the masses of a new Z boson

O. G. Miranda, V. B. Semikoz, J. W. F. Valle

Low-energy high-resolution neutrino-electron scattering experiments may play an important role in testing the gauge structure of the electroweak interaction. We discuss the use of…

hep-ph1998★ 7 cited

Radiative Neutrino Decay in Media

Dario Grasso, Victor Semikoz

In this letter we introduce a new method to determine the radiative neutrino decay rate in the presence of a medium. Our approach is based on the generalisation of the optical theo…

hep-ph1998★ 9 cited

Neutrino conversions in random magnetic fields and from the Sun

A. A. Bykov, V. Yu. Popov, A. I. Rez +2

The magnetic field in the convective zone of the Sun has a random small-scale component with the r.m.s. value substantially exceeding the strength of a regular large-scale field. F…

hep-ph1998★ 3 cited

Low-energy solar anti-neutrinos

V. B. Semikoz, S. Pastor, J. W. F. Valle

If neutrino conversions within the Sun result in partial polarization of initial solar neutrino fluxes, then a new opportunity arises to observe the anti-ν_e's in future neutrino e…

hep-ph1998

Aperiodic Spin-Flavor Conversions and from the Sun with Random Magnetic Field

V. B. Semikoz, A. A. Bykov, V. Yu. Popov +2

The magnetic field in the solar convective zone has a random small-scale component with the r.m.s. value substantially exceeding the strength of a regular large-scale field. For tw…