| Nearly bimaximal neutrino mixing, muon g-2 anomaly, and lepton-flavor-violating processes |
| Xing ZZ(邢志忠) ; Xing, ZZ
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| 2001
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发表期刊 | PHYSICAL REVIEW D
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卷号 | 64期号:1页码:17304 |
通讯作者 | Xing, ZZ (reprint author), Inst High Energy Phys, POB 918, Beijing 100039, Peoples R China.
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摘要 | We interpret the newly observed muon g-2 anomaly in the framework of a leptonic Higgs doublet model with nearly degenerate neutrino masses and nearly bimaximal neutrino mixing. Useful constraints are obtained on the rates of lepton-flavor-violating rare decays tau --> mu gamma, mu -->e gamma and tau -->e gamma well as the mu -e conversion ratio R-mue. We find that Gamma(mu -->e gamma), Gamma(tau -->e gamma) and R-mue depend crucially on possible nonzero but small values of the neutrino mixing matrix element V-e3, and they are also sensitive to the Dirac-type CP-violating phase. In particular, we show that In particular, we show that Gamma(tau --> mu gamma)/m(tau)(5), Gamma(mu -->e gamma )m(mu)(5) and Gamma(tau -->e gamma )m(tau)(5) are approximately in the ratio 1:2 \V-e3\ (2):2 \V-e3\ (2) if \ Ve3 \ is much large is much larger than O(10(-2)), and in the ratio 2(Deltam(atm)(2))(2):(Deltam(sun)(2))(2):(Deltam(sun)(2))(2) if \V-e3\ is much lower than O( 10(-3)), where Deltam(atm)(2) and Deltam(sun)(2) are the corresponding mass-squared differences of atmospheric and solar neutrino oscillations. |
文章类型 | Article
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学科领域 | Astronomy & Astrophysics; Physics
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收录类别 | SCI
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WOS类目 | Astronomy & Astrophysics
; Physics, Particles & Fields
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WOS记录号 | WOS:000169619300094
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引用统计 |
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文献类型 | 期刊论文
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条目标识符 | http://ir.ihep.ac.cn/handle/311005/227881
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专题 | 理论物理室
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推荐引用方式 GB/T 7714 |
Xing ZZ,Xing, ZZ. Nearly bimaximal neutrino mixing, muon g-2 anomaly, and lepton-flavor-violating processes[J]. PHYSICAL REVIEW D,2001,64(1):17304.
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APA |
邢志忠,&Xing, ZZ.(2001).Nearly bimaximal neutrino mixing, muon g-2 anomaly, and lepton-flavor-violating processes.PHYSICAL REVIEW D,64(1),17304.
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MLA |
邢志忠,et al."Nearly bimaximal neutrino mixing, muon g-2 anomaly, and lepton-flavor-violating processes".PHYSICAL REVIEW D 64.1(2001):17304.
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