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  • Access by Xinjiang University

Note on the neutrino mass matrix

D. C. Terry and T. K. Kuo

  • Physics Department, Purdue University, West Lafayette, Indiana 47907

Phys. Rev. D 24, 2523 – Published 1 November, 1981

DOI: https://doi.org/10.1103/PhysRevD.24.2523

Abstract

A general analysis of the Gell-Mann-Ramond-Slansky model for the neutrino mass matrix is carried out. Assuming that there is a "generation structure" for the Dirac mass matrix, and that all of the eigenvalues of the Majorana mass spectra are large, it is found that rather small neutrino mixing angles are expected.

References (4)

  1. M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by P. van Nieuwenhuizen and D. Z. Freedman (North-Holland, Amsterdam, 1979) E. Witten, Phys. Lett. 91B, 81 (1980)
  2. J. A. Harvey, P. Ramond, and D. B. Reiss, Phys. Lett. 92B, 309 (1980) in High Energy Physics—1980, proceedings of the XX International Conference, Madison, Wisconsin, edited by L. Durand and L. G. Pondron (AIP, New York, 1981) S. Hama, K. Milton, S. Nandi, and K. Tanaka, Phys. Lett. 97B, 221 (1980)
  3. K. Milton and K. Tanaka [Phys. Rev. D 23, 2087 (1981)] T. Goldman and G. J. Stephenson [ibid. 24, 236 (1981)]
  4. Omitted endnote

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