Efficient solar anti-neutrino production in random magnetic fields

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dc.creatorMiranda, O. G.
dc.creatorRashba, T. I.
dc.creatorRez, A. I.
dc.creatorValle, J. W. F.
dc.date2004-05-12
dc.date.accessioned2026-07-07T03:52:29Z
dc.date.available2026-07-07T03:52:29Z
dc.descriptionWe 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 random than regular magnetic field. This result leads to much stronger limits on the product of the neutrino transition magnetic moment and the solar magnetic field based on the recent KamLAND data. We argue that the existence of the random magnetic fields in the solar convective zone is a natural sequence of the convective zone magnetic field evolution.
dc.description7 pages, LaTeX file using JHEP3, 1 figure. Talk given by A.I.Rez at the International Workshop on Astroparticle and High Energy Physics (AHEP-2003), Valencia, Spain, 14-18 October 2003
dc.identifierhttps://arxiv.org/abs/hep-ph/0405107
dc.identifierhttp://arxiv.org/abs/hep-ph/0405107
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43481
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleEfficient solar anti-neutrino production in random magnetic fields
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