Updated CMB and x- and γ-ray constraints on Majoron dark matter

Massimiliano Lattanzi, Signe Riemer-Sørensen, Mariam Tórtola, and J. W. F. Valle
Phys. Rev. D 88, 063528 – Published 24 September 2013

Abstract

The Majoron provides an attractive dark matter candidate, directly associated with the mechanism responsible for spontaneous neutrino mass generation within the standard model SU(3)cSU(2)LU(1)Y framework. Here we update the cosmological and astrophysical constraints on Majoron dark matter coming from the cosmic microwave background and a variety of x- and γ-ray observations.

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  • Received 15 April 2013

DOI:https://doi.org/10.1103/PhysRevD.88.063528

© 2013 American Physical Society

Authors & Affiliations

Massimiliano Lattanzi1,*, Signe Riemer-Sørensen2, Mariam Tórtola3, and J. W. F. Valle3,†

  • 1Dipartimento di Fisica e Science della Terra, Università di Ferrara and INFN, sezione di Ferrara, Polo Scientifico e Tecnologico—Edificio C Via Saragat 1, I-44122 Ferrara, Italy
  • 2School of Mathematics and Physics, University of Queensland, St Lucia, Brisbane, Queensland 4072, Australia
  • 3AHEP Group, Instituto de Física Corpuscular—C.S.I.C./Universitat de València, Campus de Paterna, Apartado 22085, E–46071 València, Spain

  • *lattanzi@fe.infn.it
  • http://astroparticles.ific.uv.es

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Vol. 88, Iss. 6 — 15 September 2013

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