MHD fluctuations and low energy solar neutrinos

MHD fluctuations and low energy solar neutrinos

We analyze here how future solar neutrino experiments could detect neutrino flux fluctuations due to magnetohydrodynamics (MHD) perturbations on the solar plasma. We state that if such time fluctuations are detected, this would provide a unique signature of the resonant spin-flavor precession (RSFP)...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The European physical journal. C, Particles and fields Particles and fields, 2002-10, Vol.25 (3), p.459-464
Hauptverfasser: Guzzo, M.M., de Holanda, P.C., Reggiani, N.
Format: Artikel
Sprache:eng
Schlagworte:
Fluid dynamics
Magnetohydrodynamics
Solar neutrinos
Variation
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:We analyze here how future solar neutrino experiments could detect neutrino flux fluctuations due to magnetohydrodynamics (MHD) perturbations on the solar plasma. We state that if such time fluctuations are detected, this would provide a unique signature of the resonant spin-flavor precession (RSFP) mechanism as a solution to the solar neutrino problem.
ISSN:1434-6044
1434-6052
DOI:10.1007/s10052-002-0994-y