SOLAR-NEUTRINO EXPERIMENTS AND DETERMINATION OF THE NEUTRINO OSCILLATION PARAMETERS

被引：46

作者：

FIORENTINI, G

LISSIA, M

MEZZORANI, G

MORETTI, M

VIGNAUD, D

机构：

[1] IST NAZL FIS NUCL,I-44100 FERRARA,ITALY

[2] IST NAZL FIS NUCL,I-09127 CAGLIARI,ITALY

[3] UNIV CAGLIARI,DIPARTIMENTO SCI FIS,I-09124 CAGLIARI,ITALY

[4] INT SUPER STUDIE AVANZATI,I-34014 TRIESTE,ITALY

[5] IST NAZL FIS NUCL,I-34014 TRIESTE,ITALY

[6] CENS,DAPNIA,SERV PHYS PARTICULES,F-91191 GIF SUR YVETTE,FRANCE

来源：

PHYSICAL REVIEW D | 1994年 / 49卷 / 12期

关键词：

D O I：

10.1103/PhysRevD.49.6298

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper investigates present evidence and future tests for neutrino oscillations from solar neutrino experiments. First we analyze solar neutrino data (chlorine, Kamiokande, and gallium) in the MSW framework, including all effects that are known to influence neutrino evolution from production to detection sites, and compare our analysis with others. Next we quantitatively discuss the potential of future solar neutrino experiments (SuperKamiokande, SNO, and Borexino) for testing the MSW hypothesis, with special attention to those tests that are independent of the solar model (energy spectra, charged to neutral current ratio).

引用

页码：6298 / 6318

页数：21

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