Four-neutrino mixing and Big-Bang Nucleosynthesis

被引:42
作者
Bilenky, SM [1 ]
Giunti, C
Grimus, W
Schwetz, T
机构
[1] Joint Inst Nucl Res, Dubna, Russia
[2] Tech Univ Munich, Inst Theoret Phys, D-85748 Garching, Germany
[3] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy
[4] Univ Turin, Dipartimento Fis Teor, I-10125 Turin, Italy
[5] Univ Vienna, Inst Theoret Phys, A-1090 Vienna, Austria
关键词
D O I
10.1016/S0927-6505(99)00010-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the Big-Bang Nucleosynthesis constraints on the elements of the neutrino mixing matrix which connect sterile with massive neutrino fields, in the framework of the two four-neutrino schemes that are favored by the results of neutrino oscillation experiments, We discuss the implications of these constraints for terrestrial short and long-baseline neutrino oscillation experiments and we present several possibilities of testing them in these experiments. In particular, we show that from the Big-Bang Nucleosynthesis constraints it follows that the ((-))nu(mu) --> ((-))nu(tau) transition is severely suppressed in short-baseline experiments, whereas its oscillation amplitude in long-baseline experiments is of order i. We also propose a new parameterization of the four-neutrino mixing matrix U which is appropriate for the schemes under consideration. (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:413 / 428
页数:16
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