Built on

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Earlier work this paper cites.
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Earlier work this paper cites.
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Earlier work this paper cites.

Similar

E. Ma, Phys. Rev. Lett. 81
1998
Cited alongside, same era.
E. Ma, Phys. Rev. D66
2002
Cited alongside, same era.
K. S. Babu, E. Ma, and J. W. F. Valle, Phys. Lett. B552
2003
Cited alongside, same era.

Then

W. Grimus and L. Lavoura, Phys. Lett. B579
2004
Later among the works it cites.
S. Fraser, E. Ma, and O. Popov, Phys. Lett. B737
2014
Later among the works it cites.
Particle Data Group, K. A. Olive et al
2014
Later among the works it cites.

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2015

Neutrino Mixing and CP Phase Correlations

Ma, Ernest, Natale, Alexander, Popov, Oleg

Understand

A special form of the $3 \times 3$ Majorana neutrino mass matrix derivable from $\mu - \tau$ interchange symmetry accompanied by a generalized $CP$ transformation was obtained many years ago.

It predicts $\theta_{23} = \pi/4$ as well as $\delta_{CP} = \pm \pi/2$, with $\theta_{13} \neq 0$.
Whereas this is consistent with present data, we explore a deviation of this result which occurs naturally in a recent proposed model of radiative inverse seesaw neutrino mass.