Generalized Hidden $\mathcal{Z}_2$ Symmetry of Neutrino Mixing

B. Pontecorvo, Sov. Phys. JETP 6

1962

Earlier work this paper cites.

P. H. Frampton, S. L. Glashow and T. Yanagida, Phys. Lett. B 548

2003

Earlier work this paper cites.

V. Barger, D. A. Dicus, H. J. He and T. J. Li, Phys. Lett. B 583

2004

Earlier work this paper cites.

C. S. Lam, Phys. Rev. D74

2006

Earlier work this paper cites.

P. F. Harrison and W. G. Scott, Phys. Lett. B 547

2006

Cited alongside, same era.

G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo and A. M. Rotunno, Phys. Rev. Lett. 101

Original

2008

Cited alongside, same era.

See, for instance, the experimental reports at XXIII International Conferences on “Neutrino Physics and Astrophysics” (Neutrino 2008), Christchurch, New Zealand, May 25-31, 2008. Web link: http://www2.phys.canterbury.ac.nz/~jaa53

2008

Cited alongside, same era.

C. S. Lam, Phys. Rev. D 78

Original

2008

Cited alongside, same era.

S.- F. Ge, D. A. Dicus, and W. W. Repko, “A ℤ 2 \mathbb{Z}_{2} symmetry prediction for the Dirac C ​ P CP phase of neutrino mixing,” in preparation

Cited in the paper.

W. Grimus, L. Lavoura, P. O. Ludl, J. Phys. G G36

2009

Later among the works it cites.

P. Adamson et. al

2009

Later among the works it cites.

S.- F. Ge, H. J. He and F. R. Yin, JCAP 1005

Original

2010

Closest in time.

These conditions for one vanishing neutrino mass and k = − 1 k=-1 were derived in: D. A. Dicus, S.- F. Ge and W. W. Repko, Phys. Rev. D 82

Original

2010

Closest in time.