Built on

P. Minkowski, Phys. Lett. B 67
1979
Earlier work this paper cites.
S. F. King, Phys. Lett. B 439
2000
Earlier work this paper cites.
S. F. King, JHEP 0209
2003
Earlier work this paper cites.
S. F. King and G. G. Ross, Phys. Lett. B 520
2003
Earlier work this paper cites.
S. F. King, Phys. Rev. D 67
2003
Earlier work this paper cites.
S. F. King, JHEP 0508
2005
Earlier work this paper cites.
S. Antusch, J. Kersten, M. Lindner, M. Ratz and M. A. Schmidt, JHEP 0503
2005
Earlier work this paper cites.
S. Antusch, S. F. King and A. Riotto, JCAP 0611
2006
Earlier work this paper cites.
S. F. King, Nucl. Phys. B 786
2007
Earlier work this paper cites.
S. Antusch, S. F. King, M. Malinsky, L. Velasco-Sevilla and I. Zavala, Phys. Lett. B 666
Original
2008
Earlier work this paper cites.
S. F. King and C. Luhn, JHEP 0910
Original
2009
Earlier work this paper cites.
S. Antusch and M. Spinrath, Phys. Rev. D 79
Original
2009
Earlier work this paper cites.
G. Altarelli and F. Feruglio, Rev. Mod. Phys. 82
Original
2010
Earlier work this paper cites.

Similar

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Then

F. P. An et al
Original
2014
Closest in time.
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2014

Testing constrained sequential dominance models of neutrinos

Björkeroth, Fredrik, King, Stephen F.

Understand

Constrained sequential dominance (CSD) is a natural framework for implementing the see-saw mechanism of neutrino masses which allows the mixing angles and phases to be accurately predicted in terms of relatively few input parameters.

We analyze a class of CSD($n$) models where, in the flavour basis, two right-handed neutrinos are dominantly responsible for the "atmospheric" and "solar" neutrino masses with Yukawa couplings to $(\nu_e, \nu_{\mu}, \nu_{\tau})$ proportional to $(0,1,1)$ and $(1,n,n-2)$, respectively, where $n$ is a positive integer.
These coupling patterns may arise in indirect family symmetry models based on $A_4$.
With two right-handed neutrinos, using a $\chi^2$ test, we find a good agreement with data for CSD(3) and CSD(4) where the entire PMNS mixing matrix is controlled by a single phase $\eta$, which takes simple values, leading to accurate predictions for mixing angles and the magnitude of the oscillation phase $|\delta_{CP}|$.

Built on

P. Minkowski, Phys. Lett. B 67
1979
Earlier work this paper cites.
S. F. King, Phys. Lett. B 439
2000
Earlier work this paper cites.
S. F. King, JHEP 0209
2003
Earlier work this paper cites.
S. F. King and G. G. Ross, Phys. Lett. B 520
2003
Earlier work this paper cites.
S. F. King, Phys. Rev. D 67
2003
Earlier work this paper cites.
S. F. King, JHEP 0508
2005
Earlier work this paper cites.
S. Antusch, J. Kersten, M. Lindner, M. Ratz and M. A. Schmidt, JHEP 0503
2005
Earlier work this paper cites.
S. Antusch, S. F. King and A. Riotto, JCAP 0611
2006
Earlier work this paper cites.
S. F. King, Nucl. Phys. B 786
2007
Earlier work this paper cites.
S. Antusch, S. F. King, M. Malinsky, L. Velasco-Sevilla and I. Zavala, Phys. Lett. B 666
Original
2008
Earlier work this paper cites.
S. F. King and C. Luhn, JHEP 0910
Original
2009
Earlier work this paper cites.
S. Antusch and M. Spinrath, Phys. Rev. D 79
Original
2009
Earlier work this paper cites.
G. Altarelli and F. Feruglio, Rev. Mod. Phys. 82
Original
2010
Earlier work this paper cites.