Probability density function for neutrino masses and mixings

Jean-François Fortin, Nicolas Giasson, and Luc Marleau
Phys. Rev. D 94, 115004 – Published 1 December 2016

Abstract

The anarchy principle leading to the seesaw ensemble is studied analytically with the usual tools of random matrix theory. The probability density function for the seesaw ensemble of N×N matrices is obtained in terms of a multidimensional integral. This integral involves all light neutrino masses, leading to a complicated probability density function. It is shown that the probability density function for the neutrino mixing angles and phases is the appropriate Haar measure. The decoupling of the light neutrino masses and neutrino mixings implies no correlation between the neutrino mass eigenstates and the neutrino mixing matrix and leads to a loss of predictive power when comparing with observations. This decoupling is in agreement with some of the claims found in the literature.

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  • Received 29 September 2016

DOI:https://doi.org/10.1103/PhysRevD.94.115004

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Jean-François Fortin*, Nicolas Giasson, and Luc Marleau

  • Département de Physique, de Génie Physique et d’Optique, Université Laval, Québec City, Québec G1V 0A6, Canada

  • *jean-francois.fortin@phy.ulaval.ca
  • nicolas.giasson.1@ulaval.ca
  • luc.marleau@phy.ulaval.ca

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Issue

Vol. 94, Iss. 11 — 1 December 2016

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