Four-neutrino mass spectra and the Super-Kamiokande atmospheric up-down asymmetry

被引:113
作者
Bilenky, SM [1 ]
Giunti, C
Grimus, W
Schwetz, T
机构
[1] Joint Inst Nucl Res, Dubna, Russia
[2] Univ Vienna, Inst Theoret Phys, A-1090 Vienna, Austria
[3] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy
[4] Univ Turin, Dipartimento Fis Teor, I-10125 Turin, Italy
关键词
D O I
10.1103/PhysRevD.60.073007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the framework of schemes with mixing of four massive neutrinos, which can accommodate the atmospheric, solar and LSND ranges of Delta m(2) and contain three active neutrinos and a sterile one, we show that, in the whole region of Delta m(LSND)(2) allowed by LSND, the Super-Kamiokande up-down asymmetry excludes all mass spectra with a group of three close neutrino masses separated from the fourth mass by the LSND gap of order 1 eV. Only two schemes with mass spectra in which two pairs of close masses ore separated by the LSND gap can describe the Super-Kamiokande up-down asymmetry and all other existing neutrino oscillation data. [S0556-2821(99)03419-0].
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