2005/08/23 by S. T. Petcov, Tetsuo Shindou, T. Shindou +1 · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #CP violation #Electron #Lepton #MAJORANA #Mass matrix #Minimal Supersymmetric Standard Model #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Pontecorvo–Maki–Nakagawa–Sakata matrix #Sterile neutrino #Supersymmetry #Yukawa potential #hep-ph
paper · pdf · doi:10.1016/j.nuclphysb.2005.12.028
published as Nucl.Phys.B738:219-242,2006 · 26 pages, 5 figures
arxiv created 2005/08/23 · openalex publication_date 2006/01/23 · arxiv updated 2014/11/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We consider the MSSM with see-saw mechanism of neutrino mass generation and soft SUSY breaking with flavour-universal boundary conditions at the GUT scale, in which the lepton flavour violating (LFV) decays μ→ e + γ, τ→ μ+ γ, etc.,are predicted with rates that can be within the reach of present and planned experiments. These predictions depend critically on the matrix of neutrino Yukawa couplings \bfYν which can be expressed in terms of the light and heavy right-handed (RH) neutrino masses, neutrino mixing matrix UPMNS, and an orthogonal matrix \bfR. We investigate the effects of Majorana CP-violation phases in UPMNS, and of the RG running of light neutrino masses and mixing angles from MZ to the RH Majorana neutrino mass scale MR, on the predictions for the rates of LFV decays μ→ e + γ, τ→ μ+ γand τ→ e + γ. Results for neutrino mass spectrum with normal hierarchy, values of the lightest ν-mass in the range 0 ≤ m1 ≤ 0.30 eV, and quasi-degenerate heavy RH Majorana neutrinos in the cases of \bfR = \bf1 and complex matrix \bfR are presented. We find that the effects of the Majorana CP-violation phases and of the RG evolution of neutrino mixing parameters can change by few orders of magnitude the predicted rates of the LFV decays μ→ e + γand τ→ e + γ. The impact of these effects on the τ→ μ+ γdecay rate is typically smaller and only possible for m1 > 0.10 eV. If the RG running effects are negligible, in a large region of soft SUSY breaking parameter space the ratio of the branching ratios of the μ→ e + γand τ→ e + γ(τ→ μ+ γ) decays is entirely determined in the case of \bfR ≅ \bf1 by the values of the neutrino mixing parameters at MZ.