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      Muon anomalous magnetic moment, lepton flavor violation, and flavor changing neutral current processes in SUSY GUT with right-handed neutrino

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          Abstract

          Motivated by the large mixing angle solutions for the atmospheric and solar neutrino anomalies, flavor changing neutral current processes and lepton flavor violating processes as well as the muon anomalous magnetic moment are analyzed in the framework of SU(5) SUSY GUT with right-handed neutrino. In order to explain realistic mass relations for quarks and leptons, we take into account effects of higher dimensional operators above the GUT scale. It is shown that the supersymmetric (SUSY) contributions to the CP violation parameter in \(K^0-\bar{K}^0\) mixing, \(\epsilon_K\), the \(\mu \to e \gamma\) branching ratio, and the muon anomalous magnetic moment become large in a wide range of parameter space. We also investigate correlations among these quantities. Within the current experimental bound of \(\text{B}(\mu \to e \gamma)\), large SUSY contributions are possible either in the muon anomalous magnetic moment or in \(\epsilon_K\). In the former case, the favorable value of the recent muon anomalous magnetic moment measurement at the BNL E821 experiment can be accommodated. In the latter case, the allowed region of the Kobayashi-Maskawa phase can be different from the prediction within the Standard Model (SM) and therefore the measurements of the CP asymmetry of \(B\to J/\psi K_S\) mode and \(\Delta m_{B_s}\) could discriminate this case from the SM. We also show that the \(\tau \to \mu \gamma\) branching ratio can be close to the current experimental upperbound and the mixing induced CP asymmetry of the radiative B decay can be enhanced in the case where the neutrino parameters correspond to the Mikheyev-Smirnov-Wolfenstein small mixing angle solution.

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          Muon Decay and Physics Beyond the Standard Model

          This article reviews the current theoretical and experimental status of the field of muon decay and its potential to search for new physics beyond the Standard Model. The importance of rare muon processes with lepton flavor violation is highly stressed, together with precision measurements of normal muon decay. Recent up-to-date motivations of lepton flavor violation based on supersymmetric models, in particular supersymmetric grand unified theories, are described along with other theoretical models. Future prospects of experiments and muon sources of high intensity for further progress in this field are also discussed.
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            Solar and Atmospheric Neutrino Oscillations and Lepton Flavor Violation in Supersymmetric Models with Right-handed Neutrinos

            , (2009)
            Taking the solar and the atmospheric neutrino experiments into account we discuss the lepton flavor violating processes, such as \(\tau\to\mu\gamma\) or \(\mu\to e\gamma\), in the minimal supersymmetric standard model with right-handed neutrinos (MSSMRN) and the supersymmetric SU(5) GUT with right-handed neutrinos (SU(5)RN). The predicted branching ratio of \(\mu\to e\gamma\) in the MSSMRN with the MSW large angle solution is so large that it goes beyond the current experimental bound if the second-generation right-handed Majorana mass \(M_{\nu_2}\) is greater than \(\sim 10^{13}(\sim 10^{14})\)GeV for \(\tan\beta=30(3)\). When we take the MSW small angle solution, the \(\mu\to e\gamma\) rate is at most about 1/100 of that of the MSW large angle solution. The 'just so' solution implies \(10^{-5}\) of that of the MSW large angle solution. Also, in the SU(5)RN the large \(\mu\to e\gamma\) rate naturally follows from the MSW large angle solution, and the predicted rate is beyond the current experimental bound if the typical right-handed Majorana mass \(M_N\) is larger than \(\sim 10^{13}(\sim 10^{14})\)GeV for \(\tan\beta=30(3)\), similarly to the MSSMRN. We show the multimass insertion formulas and their applications to \(\tau\to\mu\gamma\) and \(\mu\to e\gamma\).
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              Anomaly mediation in supergravity theories

              We consider the effects of anomalies on the supersymmetry-breaking parameters in supergravity theories. We construct a supersymmetric expression for the anomaly-induced terms in the 1PI effective action; we use this result to compute the complete one-loop formula for the anomaly-induced gaugino mass. The mass receives contributions from the super-Weyl, Kahler, and sigma-model anomalies of the supergravity theory. We point out that the anomaly-mediated gaugino mass can be affected by local counterterms that cancel the super-Weyl-Kahler anomaly. This implies that the gaugino mass cannot be predicted unless the full high-energy theory is known.
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                Author and article information

                Journal
                2001-04-16
                Article
                10.1103/PhysRevD.64.095001
                hep-ph/0104146
                070a8aa0-ce76-4989-aa17-4214da51c223
                History
                Custom metadata
                KEK-TH-760, ICRR-Report-476-2001-6
                Phys.Rev. D64 (2001) 095001
                70 pages, 14 figures
                hep-ph

                High energy & Particle physics
                High energy & Particle physics

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