What will the first year of SNO show?

被引:43
作者
Bahcall, JN
Krastev, PI
Smirnov, AY
机构
[1] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA
[2] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[3] Int Ctr Theoret Phys, I-34100 Trieste, Italy
基金
美国国家科学基金会;
关键词
D O I
10.1016/S0370-2693(00)00250-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ratio of the measured to the predicted standard model CC event rates in SNO will be 0.47 if no oscillations occur. The best-fit active oscillation predictions for the CC ratio are: 0.35-39 (MSW) and 0.38-42 (vacuum) (all for a 5 MeV energy threshold), typically about 20% less than the no-oscillation expectation. We calculate the predicted ratios for six active and sterile neutrino oscillation solutions allowed at 99% CL and determine the dependence of the ratios on energy threshold. If the high-energy anomaly observed by SuperKamiokande is due to an enhanced hep flux, MSW active solutions predict that out of a total of 5000 CC events above 5 MeV in SNO between 49 and 54 events will be observed above 13 MeV whereas only 19 events are expected for no-oscillations and a nominal standard hep flux. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
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页码:401 / 409
页数:9
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