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Original
1959
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B. Pontecorvo, Sov. Phys. JETP 26 (1968) 984 [Zh. Eksp. Teor. Fiz. 53 (1967) 1717]; Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys. 28 (1962) 870
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L.M. Krauss, S. Nasri and M. Trodden, Phys. Rev. D 67 (2003) 085002, arXiv:hep-ph/0210389
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K. Cheung and O. Seto, Phys. Rev. D 69 (2004) 113009, arXiv:hep-ph/0403003
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R. Barbieri, L.J. Hall and V.S. Rychkov, Phys. Rev. D 74 (2006) 015007, arXiv:hep-ph/0603188
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2015

A three-loop radiative neutrino mass model with dark matter

Jin, Li-Gang, Tang, Rui, Zhang, Fei

Understand

We present a model that generates small neutrino masses at three-loop level due to the existence of Majorana fermionic dark matter, which is stabilized by a Z2 symmetry.

The model predicts that the lightest neutrino is massless.
We show a prototypical parameter choice allowed by relevant experimental data, which favors the case of normal neutrino mass spectrum and the dark matter with m \sim 50-135 GeV and a sizable Yukawa coupling.
It means that new particles can be searched for in future e+e- collisions.

Built on

A. Freitas and S. Westhoff, arXiv:1408.1959 [hep-ph]
Original
1959
Earlier work this paper cites.
B. Pontecorvo, Sov. Phys. JETP 26 (1968) 984 [Zh. Eksp. Teor. Fiz. 53 (1967) 1717]; Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys. 28 (1962) 870
1962
Earlier work this paper cites.
L.M. Krauss, S. Nasri and M. Trodden, Phys. Rev. D 67 (2003) 085002, arXiv:hep-ph/0210389
2003
Earlier work this paper cites.
E.A. Baltz and L. Bergstrom, Phys. Rev. D 67 (2003) 043516, arXiv:hep-ph/0211325
2003
Earlier work this paper cites.
K. Cheung and O. Seto, Phys. Rev. D 69 (2004) 113009, arXiv:hep-ph/0403003
2004
Earlier work this paper cites.
E. Ma, Phys. Rev. D 73 (2006) 077301, arXiv:hep-ph/0601225
2006
Earlier work this paper cites.
R. Barbieri, L.J. Hall and V.S. Rychkov, Phys. Rev. D 74 (2006) 015007, arXiv:hep-ph/0603188
2006
Earlier work this paper cites.