τ→μγ and μ→eγ as probes of neutrino mass models

被引:119
作者
Lavignac, S [1 ]
Masina, I
Savoy, CA
机构
[1] CEA Saclay, Serv Phys Theor, Lab Direct Sci Mat, F-91191 Gif Sur Yvette, France
[2] CEA Saclay, Serv Phys Theor, URA CNRS 2306, F-91191 Gif Sur Yvette, France
关键词
D O I
10.1016/S0370-2693(01)01111-X
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the possibility of discriminating between different supersymmetric see-saw models by improving the experimental sensitivity to charged lepton flavour violating processes. Assuming a hierarchical neutrino mass spectrum, we classify see-saw models according to how the hierarchy Deltam(circle dot)(2) much less than Deltam(atm)(2) is generated, and study the predictions of each class for the branching ratios of tau --> mu gamma and mu --> e gamma. The process tau --> mu gamma is found to be a particularly promising tool to probe the fundamental seesaw parameters, and especially to identify the origin of the large atmospheric mixing angle. Predictions for mu --> e gamma are more model-dependent. We point out that, even with an improvement of the experimental sensitivities by three orders of magnitude, both tau --> mu gamma and mu --> e gamma could escape detection in models where Deltam(atm)(2) is determined by one of the lightest right-handed atm neutrinos. (C) 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:269 / 278
页数:10
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