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I comment on the proposal that the stability of dark matter may be due to an unbroken Z_2 symmetry contained in the partially broken lepton flavour symmetry group.
For instance, W. Grimus and L. Lavoura, “Seesaw model with softly broken L e − L μ − L τ L_{e}-L_{\mu}-L_{\tau} ,” JHEP
2000
Earlier work this paper cites.
W. Grimus and L. Lavoura, “One-loop corrections to the seesaw mechanism in the multi-Higgs-doublet standard model,” Phys. Lett. B
2002
Earlier work this paper cites.
The notation for the neutral scalars is detailed in W. Grimus and H. Neufeld, “Radiative neutrino masses in an SU(2) × \times U(1) model,” Nucl. Phys. B
2002
Earlier work this paper cites.
D 4 D_{4} has been used as lepton flavour symmetry group in W. Grimus and L. Lavoura, “A discrete symmetry group for maximal atmospheric neutrino mixing,” Phys. Lett. B
2003
Earlier work this paper cites.
L. Lavoura, “Zeros of the inverted neutrino mass matrix,” Phys. Lett. B
2005
Cited alongside, same era.
E. Ma, “Verifiable radiative seesaw mechanism of neutrino mass and dark matter,” Phys. Rev. D
2006
Cited alongside, same era.
The D n D_{n} groups have been discussed in detail in A. Blum, C. Hagedorn, and M. Lindner, “Fermion masses and mixings from dihedral flavor symmetries with preserved subgroups,” Phys. Rev. D
2008
Cited alongside, same era.
W. Grimus, A. S. Joshipura, S. Kaneko, L. Lavoura, H. Sawanaka, and M. Tanimoto, “Non-vanishing U e 3 U_{e3} and cos 2 θ 23 \cos{2\theta_{23}} from a broken ℤ 2 \mathbbm{Z}_{2} symmetry,” Nucl. Phys. B
Cited in the paper.
P. O. Ludl, private communication
Cited in the paper.
Cited in the paper.
W. Grimus, L. Lavoura, and P. O. Ludl, “Is S 4 S_{4} the horizontal symmetry of tri-bimaximal lepton mixing?,” J. Phys. G
2009
Later among the works it cites.
M. Hirsch, S. Morisi, E. Peinado, and J. W. F. Valle, “Discrete dark matter,” Phys. Rev. D
2010
Later among the works it cites.
D. Meloni, S. Morisi, and E. Peinado, “Neutrino phenomenology and stable dark matter with A 4 A_{4} ,” Phys. Lett. B
2011
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