Study of the day-night effect for the Super-Kamiokande detector .2. Electron spectrum deformations and day-night asymmetries

被引:53
|
作者
Maris, M
Petcov, ST
机构
[1] IST NAZL FIS NUCL, SEZ PAVIA, I-27100 PAVIA, ITALY
[2] BULGARIAN ACAD SCI, INST NUCL RES & NUCL ENERGY, BU-1784 SOFIA, BULGARIA
关键词
D O I
10.1103/PhysRevD.56.7444
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using the results of a high precision calculation of the solar neutrino survival probability for Earth crossing neutrinos in the case of the MSW nu(e) --> nu(mu(tau)) transition solution of the solar neutrino problem, performed in an earlier study, we derive predictions for the one-year-averaged day-night (D-N) asymmetry in the deformations of the e(-) spectrum to be measured with the Super-Kamiokande detector, and for the D-N asymmetry in the energy-integrated one-year signal in this detector. The asymmetries are calculated for the solar nu(e) crossing the Earth mantle only, the core, and the (mantle+core) for a large representative set of values of the MSW transition parameters Delta m(2) and sin(2) 2 theta(V) from the ''conservative'' MSW solution region obtained by taking into account possible uncertainties in the values of the B-8 and Be-7 neutrino fluxes. The effect of the uncertainties in the value of the bulk matter density and in the chemical composition of the core on the D-N asymmetry predictions is studied. It is shown, in particular, that for sin(2) 2 theta V less than or equal to 0.013 the one-year average D-N asymmetry for neutrinos crossing the Earth core can be larger than the asymmetry for (only mantle crossing+core crossing) neutrinos by a factor of up to six. Iso-(D-N) asymmetry contours in the Delta m(2) - sin(2) 2 theta(V) plane for the Super-Kamiokande detector are derived in the region sin(2) 2 theta(V) greater than or similar to 10(-4) for only mantle crossing, core crossing, and (only mantle crossing+core crossing) neutrinos. The dependence of the D-N asymmetry in the three data samples on the recoil-e(-) energy threshold is also investigated. Our results indicate that the Super-Kamiokande experiment might be able to test the sin(2) 2 theta(V) less than or equal to 0.01 region of the MSW solution of the solar neutrino problem by performing selective D-N asymmetry measurements.
引用
收藏
页码:7444 / 7455
页数:12
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