Patterns of lepton-flavour violation motivated by decoupling and sneutrino inflation
We present predictions for flavour-violating charged-lepton decays induced by the seesaw mechanism implemented within the constrained minimal supersymmetric standard model (CMSSM) with universal input soft supersymmetry breaking terms. We assume that one heavy singlet neutrino almost decouples from...
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| Published in | Nuclear physics. B Vol. 690; no. 3; pp. 279 - 301 |
|---|---|
| Main Authors | , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Elsevier B.V
12.07.2004
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| Subjects | |
| Online Access | Get full text |
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| Abstract | We present predictions for flavour-violating charged-lepton decays induced by the seesaw mechanism implemented within the constrained minimal supersymmetric standard model (CMSSM) with universal input soft supersymmetry breaking terms. We assume that one heavy singlet neutrino almost decouples from the seesaw mechanism, as suggested by the pattern of light neutrino masses and mixing angles. This is suggested independently by sneutrino inflation with a low reheating temperature,
T
RH
≲10
7
GeV
, so as to avoid overproducing gravitinos. This requirement further fixes the mass of the weakly-coupled sneutrino, whose decays may lead to leptogenesis. We find that
BR(
μ→
eγ)≳10
−13 but
BR(
τ→
μγ)≲10
−9 in the bulk of the acceptable parameter space, apart from a few isolated points. The ratio
BR(
μ→
eγ)/
BR(
τ→
eγ) depends on only one complex parameter, and is particularly interesting to compare with experiment. |
|---|---|
| AbstractList | We present predictions for flavour-violating charged-lepton decays induced by the seesaw mechanism implemented within the constrained minimal supersymmetric standard model (CMSSM) with universal input soft supersymmetry breaking terms. We assume that one heavy singlet neutrino almost decouples from the seesaw mechanism, as suggested by the pattern of light neutrino masses and mixing angles. This is suggested independently by sneutrino inflation with a low reheating temperature,
T
RH
≲10
7
GeV
, so as to avoid overproducing gravitinos. This requirement further fixes the mass of the weakly-coupled sneutrino, whose decays may lead to leptogenesis. We find that
BR(
μ→
eγ)≳10
−13 but
BR(
τ→
μγ)≲10
−9 in the bulk of the acceptable parameter space, apart from a few isolated points. The ratio
BR(
μ→
eγ)/
BR(
τ→
eγ) depends on only one complex parameter, and is particularly interesting to compare with experiment. |
| Author | Chankowski, Piotr H. Pokorski, Stefan Turzyński, Krzysztof Ellis, John Raidal, Martti |
| Author_xml | – sequence: 1 givenname: Piotr H. surname: Chankowski fullname: Chankowski, Piotr H. organization: Institute of Theoretical Physics, Warsaw University, Hoża 69, 00-681 Warsaw, Poland – sequence: 2 givenname: John surname: Ellis fullname: Ellis, John organization: Theoretical Physics Division, Physics Department, CERN, CH-1211 Geneva 23, Switzerland – sequence: 3 givenname: Stefan surname: Pokorski fullname: Pokorski, Stefan organization: Institute of Theoretical Physics, Warsaw University, Hoża 69, 00-681 Warsaw, Poland – sequence: 4 givenname: Martti surname: Raidal fullname: Raidal, Martti organization: National Institute of Chemical Physics and Biophysics, Tallinn 10143, Estonia – sequence: 5 givenname: Krzysztof surname: Turzyński fullname: Turzyński, Krzysztof email: krzysztof-jan.turzynski@fuw.edu.pl organization: Institute of Theoretical Physics, Warsaw University, Hoża 69, 00-681 Warsaw, Poland |
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662 Buchmüller (10.1016/j.nuclphysb.2004.05.001_BIB005_1) 2002; 643 Akhmedov (10.1016/j.nuclphysb.2004.05.001_BIB008_7) 2003; 0309 Pilaftsis (10.1016/j.nuclphysb.2004.05.001_BIB049) Feng (10.1016/j.nuclphysb.2004.05.001_BIB036_3) 2000; 61 Ellis (10.1016/j.nuclphysb.2004.05.001_BIB009) 2002; 643 Peiris (10.1016/j.nuclphysb.2004.05.001_BIB018_3) 2003; 148 Altarelli (10.1016/j.nuclphysb.2004.05.001_BIB014_2) 2003 Petcov (10.1016/j.nuclphysb.2004.05.001_BIB025_2) 2004; 676 King (10.1016/j.nuclphysb.2004.05.001_BIB013_3) 1999; 562 King (10.1016/j.nuclphysb.2004.05.001_BIB013_10) 2001; 520 Kuchimanchi (10.1016/j.nuclphysb.2004.05.001_BIB034_1) 2002; 66 Yanagida (10.1016/j.nuclphysb.2004.05.001_BIB003_2) 1979 Hall (10.1016/j.nuclphysb.2004.05.001_BIB002_2) 1986; 267 King (10.1016/j.nuclphysb.2004.05.001_BIB013_6) 2004; 67 Ellis (10.1016/j.nuclphysb.2004.05.001_BIB041_1) 2003; 565 Branco (10.1016/j.nuclphysb.2004.05.001_BIB012) 2003; 67 Turzynski (10.1016/j.nuclphysb.2004.05.001_BIB052) 2004; 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