Current status of the resonant spin-flavor precession solution to the solar neutrino problem

被引:51
作者
Guzzo, MM [1 ]
Nunokawa, H [1 ]
机构
[1] Univ Estadual Campinas, Inst Fis Gleb Wataghin, BR-13083970 Campinas, SP, Brazil
基金
巴西圣保罗研究基金会;
关键词
D O I
10.1016/S0927-6505(99)00075-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the current status of the resonant spin-flavor precession (RSFP) solution to the solar neutrino problem. We perform a fit to all the latest solar neutrino data for various assumed magnetic field profiles in the Sun. We show that the RSFP can account for all the solar neutrino experiments, giving as good a fit as other alternative solutions such as MSW or vacuum oscillation (Just So), and therefore can be a viable solution to the solar neutrino problem (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:87 / 95
页数:9
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