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On fitting the type II seesaw mechanism into the type I seesaw mechanism, we obtain a formula to the neutrino masses which get suppressed by high-scale $M^3$ in its denominator.
For type I seesaw mechanism, see Refs.: M. Gell-Mann, P. Ramond, and R. Slansky, in supergravity
1980
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R. Foot, H. N. Long and T. A. Tran, Phys. Rev. D 50
1993
Earlier work this paper cites.
For type II seesaw mechanism, see Refs.: M. Magg, C. Wetterich, Phys. Lett. B 94
1998
Earlier work this paper cites.
For type III seesaw mechanism, see ref.: R. Foot, H. Lew, X. G. He, G. C. Joshi, Z. Phys. C 44
1998
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Ernest Ma, Phys. Rev. Lett. 86
2001
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SNO Collaboration (Q. R. Ahmad et al
2002
Cited alongside, same era.
KamLAND Collaboration (K. Eguchi et al
2003
Cited alongside, same era.
K2K Collaboration (M. H. Ahn et al
2003
Cited alongside, same era.
C. A. de S.Pires, P. S. Rodrigues da Silva, Eur. Phys. J. C 36
2004
Cited alongside, same era.
Super-Kamiokande Collaboration (J. Hosaka et al
2006
Cited alongside, same era.
2007
Later among the works it cites.
This scalar sextet was first introduced in the second paper in Ref. [ 11 ] . Recently it was reintroduced in Refs.: N. A. Ky, N. T. H. Van, Phys. Rev. D 72
2008
Later among the works it cites.
W. Grimus, L. Lavoura, B. Radovcic, Phys. Lett. B 674
2009
Later among the works it cites.
The type II seesaw mechanism in a version of the 3-3-1 models called the minimal 3-3-1 model was implemented in the refs.: J. C. Montero, C. A. de S. Pires, V. Pleitez, Phys. Lett. B 502
2009
Later among the works it cites.
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