Probing the LSND mass scale and four neutrino scenarios with a neutrino telescope

被引:70
|
作者
Nunokawa, H
Peres, OLG
Funchal, RZ
机构
[1] Univ Estadual Paulista, Inst Fis Teor, BR-01405900 Sao Paulo, Brazil
[2] Univ Calif Santa Barbara, Kavil Inst Theoret Phys, Santa Barbara, CA 93106 USA
[3] Univ Estadual Campinas, UNICAMP, Inst Fis Gleb Wataghin, BR-13083970 Campinas, SP, Brazil
[4] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
关键词
D O I
10.1016/S0370-2693(03)00603-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show in this Letter that the observation of the angular distribution of upward-going muons and cascade events induced by atmospheric neutrinos at the TeV energy scale, which can be performed by a kilometer-scale neutrino telescope, such as the IceCube detector, can be used to probe a large neutrino mass splitting, \Deltam(2)\ similar to (0.5-2.0) eV(2), implied by the LSND experiment and discriminate among four neutrino mass schemes. This is due to the fact that such a large mass scale can promote non-negligible nu(mu) --> nu(e), nu(tau)/(nu(mu)) over bar --> (nu(e)) over bar,(nu(tau)) over bar conversions at these energies by the MSW effect as well as vacuum oscillation, unlike what is expected if all the neutrino mass splittings are small. (C) 2003 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:279 / 290
页数:12
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