Understand
Assuming that neutrinos acquire radiative seesaw Majorana masses through their interactions with dark matter, i.e.
- scotogenic from the Greek 'scotos' meaning darkness, and using the non-Abelian discrete symmetry $A_4$, we propose a model of neutrino masses and mixing with nonzero $\theta_{13}$ and necessarily large leptonic CP violation, allowing both the normal and inverted hierarchies of neutrino masses, as well as quasi-degenerate solutions.
Built on
N. G. Deshpande and E. Ma, Phys. Rev. D18
1978
Earlier work this paper cites.
E. Ma and G. Rajasekaran, Phys. Rev. D64
2001
Earlier work this paper cites.
E. Ma, Mod. Phys. Lett. A17
2002
Earlier work this paper cites.
K. S. Babu, E. Ma, and J. W. F. Valle, Phys. Lett. B552
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Earlier work this paper cites.
E. Ma, Phys. Rev. D70
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Earlier work this paper cites.
Similar
E. Ma, Phys. Rev. D73
2006
Cited alongside, same era.
E. Ma, Phys. Rev. D82
2010
Cited alongside, same era.
Particle Data Group: K. Nakamura et al
2010
Cited alongside, same era.
Q.-H. Cao, S. Khalil, E. Ma, and H. Okada, Phys. Rev. Lett. 106
2011
Cited alongside, same era.
H. Ishimori and E. Ma, arXiv:1205.0075 [hep-ph]
Cited in the paper.
Then
Q.-H. Cao, A. Damanik, E. Ma, and D. Wegman, Phys. Rev. D83
2011
Later among the works it cites.
E. Ma and D. Wegman, Phys. Rev. Lett. 107
2011
Later among the works it cites.
Daya Bay Collaboration: F. P. An et al
2012
Closest in time.
RENO Collaboration: J. K. Ahn et al
2012
Closest in time.
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