期刊
PHYSICS LETTERS B
卷 695, 期 5, 页码 476-481出版社
ELSEVIER
DOI: 10.1016/j.physletb.2010.11.063
关键词
Non-Abelian discrete symmetry; Decaying dark matter; Cosmic-ray measurement
资金
- Ministry of Education, Science, Sports, and Culture of Japan [20244028, 20540272, 20740135, 21740174, 22011005, 22244021, 22244031]
- grant-in-aid for the global COE program
- ESF [8090]
- Science and Technology Development Fund (STDF) [ID 437]
- ICTP [ID 30]
- Grants-in-Aid for Scientific Research [22011005, 20740135] Funding Source: KAKEN
The positron anomaly recently reported by the cosmic-ray measurements can be explained by the decaying dark matter scenario, where it decays mainly into leptons with the lifetime of O(10(26)) s. When the dark matter is a fermionic particle, the lifetime of this order is known to be obtained by a dimension 6 operator suppressed by the unification scale (similar to 10(16) GeV), while such decay operators do not necessarily involve only leptons. In addition, the scenario would be spoiled if there exist lower-dimensional operators inducing the dark matter decay. We show in this Letter that a single non-Abelian discrete symmetry such as A(4) is possible to prohibit all such harmful (non-leptonically coupled and lower-dimensional) operators. Moreover, the dark matter decays into charged leptons in a flavor-blind fashion due to the non-Abelian flavor symmetry, which results in perfect agreements not only with the PAMELA data but also with the latest Fermi-LAT data reported very recently. We also discuss some relevance between the discrete symmetry and neutrino physics. (C) 2010 Elsevier BM. All rights reserved.
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