MHD fluctuations and low energy solar neutrinos

被引：1
|
作者：
Guzzo, MM [1 ]
de Holanda, PC
Reggiani, N
机构：
[1] Univ Estadual Campinas, UNICAMP, Inst Fis Gleb Wataghin, BR-13083970 Campinas, SP, Brazil
[2] Pontificia Univ Catolica Campinas, Fac Matemat, Ctr Ciencias Exatas Ambientais & Tecnol, BR-13086900 Campinas, SP, Brazil
来源：
EUROPEAN PHYSICAL JOURNAL C | 2002年 / 25卷 / 03期
关键词：
D O I：
10.1007/s10052-002-0994-y
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
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.
引用
收藏
页码：459 / 464
页数：6
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