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Resonant spin-flavor precession of solar and supernova neutrinos
Abstract
The combined effect of matter and magnetic fields on neutrino spin and flavor precession is examined. We find a potential new kind of resonant or (for Dirac neutrinos) or ${\ensuremath{\nu}}_{e}$\ensuremath{\rightarrow}\ensuremath{\nu}${\ifmmode\bar\else\textasciimacron\fi{}}_{\ensuremath{\mu}}$ or \ensuremath{\nu}${\ifmmode\bar\else\textasciimacron\fi{}}_{\ensuremath{\tau}}$ (for Majorana neutrinos). Such a resonance could help account for the lower than expected solar-neutrino ${\ensuremath{\nu}}_{e}$ flux and/or indications of an anticorrelation between fluctuations in the ${\ensuremath{\nu}}_{e}$ flux and sunspot activity. Consequences of spin-flavor precession for supernova neutrinos are also briefly discussed.
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Cited by
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Barbier, R., Bérat, C., Besançon, M., Chemtob, M., Deandrea, A., Dudas, E., Fayet, P., Lavignac, S., Moreau, G., Perez, E., et al. (2005) · Physics Reports · doi:10.1016/j.physrep.2005.08.006 · Cited by 1,043
Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties
Bahcall, J. N., Pinsonneault, M. H., & Basu, S. (2001) · The Astrophysical Journal · doi:10.1086/321493 · Cited by 885
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Metadata
- Authors
- Lim, C.-S., & Marciano, W. J.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1988-03-15
- Volume
- 37
- Issue
- 6
- Pages
- 1368-1373
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2015855554
- Cited by
- 439
- References
- 0
- FWCI
- 15.24
- Type
- journal article
- Language
- en
- Open access
- closed
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