activity
19942004
most citedConstraining the neutrino magnetic moment with anti-neutrinos from the Sun

67 citations · 200 across the 9 of their papers we have counts for

collaborators

8 papers

hep-ph2004★ 41 cited

Enhanced solar anti-neutrino flux in random magnetic fields

O. G. Miranda, T. I. Rashba, A. I. Rez +1

We discuss the impact of the recent KamLAND constraint on the solar anti-neutrino flux on the analysis of solar neutrino data in the presence of Majorana neutrino transition magnet…

hep-ph2004

Efficient solar anti-neutrino production in random magnetic fields

O. G. Miranda, T. I. Rashba, A. I. Rez +1

We have shown that the electron anti-neutrino appearance in the framework of the spin flavor conversion mechanism is much more efficient in the case of neutrino propagation through…

hep-ph2003★ 67 cited

Constraining the neutrino magnetic moment with anti-neutrinos from the Sun

O. G. Miranda, T. I. Rashba, A. I. Rez +1

We discuss the impact of different solar neutrino data on the spin-flavor-precession (SFP) mechanism of neutrino conversion. We find that, although detailed solar rates and spectra…

hep-ph2002

Gauge invariance and weak forces in an isotropic medium

A. I. Rez, V. B. Semikoz

We demonstrate that the neutrino kinetic equation derived by the standard Bogolyubov method is formally gauge non-invariant and give a recipe how to recast it to the gauge invarian…

hep-ph1999

Neutrino Spin-Flavor Conversions and Electron Antineutrino emission 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 substancially exceeding the strength of a regular large-scale field. For tw…

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…