• Rapid Communication

High scale mixing unification for Dirac neutrinos

Gauhar Abbas, Saurabh Gupta, G. Rajasekaran, and Rahul Srivastava
Phys. Rev. D 91, 111301(R) – Published 25 June 2015

Abstract

Starting with the high scale mixing unification hypothesis, we investigate the renormalization-group evolution of mixing parameters and masses for Dirac-type neutrinos. Following this hypothesis, the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) mixing angles and phase are taken to be identical to the Cabibbo-Kobayashi-Maskawa (CKM) ones at a unifying high scale. Then they are evolved to a low scale using renormalization-group equations. The notable feature of this hypothesis is that renormalization-group evolution with quasidegenerate mass pattern can explain largeness of leptonic mixing angles even for Dirac neutrinos. The renormalization-group evolution “naturally” results in a nonzero and small value of leptonic mixing angle θ13. One of the important predictions of this work is that the mixing angle θ23 is nonmaximal and lies only in the second octant. We also derive constraints on the allowed parameter range for the supersymmetry breaking and unification scales for which this hypothesis works. The results are novel and can be tested by present and future experiments.

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  • Received 14 January 2014

DOI:https://doi.org/10.1103/PhysRevD.91.111301

© 2015 American Physical Society

Authors & Affiliations

Gauhar Abbas1,*, Saurabh Gupta1,†, G. Rajasekaran1,2,‡, and Rahul Srivastava1,§

  • 1The Institute of Mathematical Sciences, Chennai 600 113, Tamil Nadu, India
  • 2Chennai Mathematical Institute, Siruseri 603 103, Tamil Nadu, India

  • *Gauhar.Abbas@ific.uv.es
  • Present address: Instituto de Física, Universidade de São Paulo, C. Postal 66318, 05314-970 São Paulo, SP, Brazil. saurabh@if.usp.br
  • graj@imsc.res.in
  • §rahuls@imsc.res.in

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Issue

Vol. 91, Iss. 11 — 1 June 2015

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