MHD solar fluctuations and solar neutrinos

被引：0
|
作者：
Reggiani, N [1 ]
Guzzo, MM
de Holanda, PC
机构：
[1] Pontificia Univ Catolica Campinas, Fac Matemat, Ctr Ciencias Exatas Ambientais & Tecnol, BR-13086900 Campinas, SP, Brazil
[2] Univ Estadual Campinas, Inst Fis Gleb Wataghin, UNICAMP, BR-13083970 Campinas, SP, Brazil
[3] Abdus Salam Int Ctr Theoret Phys, I-34100 Trieste, Italy
来源：
BRAZILIAN JOURNAL OF PHYSICS | 2003年 / 33卷 / 04期
关键词：
D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamic (MHD) perturbations of 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.
引用
收藏
页码：767 / 774
页数：8
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