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2016

Dark matter and observable Lepton Flavour Violation

Heurtier, Lucien, Teresi, Daniele

Understand

Seesaw models with leptonic symmetries allow right-handed (RH) neutrino masses at the electroweak scale, or even lower, at the same time having large Yukawa couplings with the Standard Model leptons, thus yielding observable effects at current or near-future lepton-flavour-violation (LFV) experiments.

These models have been previously considered also in connection to low-scale leptogenesis, but the combination of observable LFV and successful leptogenesis has appeared to be difficult to achieve unless the leptonic symmetry is embedded into a larger one.
In this paper, instead, we follow a different route and consider a possible connection between large LFV rates and Dark Matter (DM).
We present a model in which the same leptonic symmetry responsible for the large Yukawa couplings guarantees the stability of the DM candidate, identified as the lightest of the RH neutrinos.

Built on

A. Pilaftsis, Phys. Rev. D 49
Original
1919
Earlier work this paper cites.
S. Tremaine and J. E. Gunn, Phys. Rev. Lett. 42
1979
Earlier work this paper cites.
H. Fritzsch and P. Minkowski, Annals Phys. 93
1979
Earlier work this paper cites.
P. Minkowski, Phys. Lett. B 67
Original
1980
Earlier work this paper cites.
Y. Chikashige, R. N. Mohapatra and R. D. Peccei, Phys. Lett. B 98
1981
Earlier work this paper cites.
R. N. Mohapatra, Phys. Rev. Lett. 56
1986
Earlier work this paper cites.
Y. Farzan, Phys. Rev. D 67
1988
Earlier work this paper cites.
A. Pilaftsis, Z. Phys. C 55
1992
Earlier work this paper cites.
Y. Farzan, Phys. Rev. D 67
2003
Earlier work this paper cites.
A. Pilaftsis, Phys. Rev. D 56
2004
Earlier work this paper cites.
T. Asaka, S. Blanchet and M. Shaposhnikov, Phys. Lett. B 631
2005
Earlier work this paper cites.
S. M. Barr, Phys. Rev. Lett. 92
2005
Earlier work this paper cites.