Gravitino dark matter and neutrino masses in partial split supersymmetry

Marco Aurelio Díaz, Sebastián García Sáenz, and Benjamin Koch
Phys. Rev. D 84, 055007 – Published 12 September 2011

Abstract

Partial split supersymmetry with bilinear R-parity violation allows one to reproduce all neutrino mass and mixing parameters. The viable dark matter candidate in this model is the gravitino. We study the hypothesis that both possibilities are true: partial split supersymmetry explains neutrino physics and dark matter is actually composed of gravitinos. Since the gravitino has a small but nonzero decay probability, its decay products could be observed in astrophysical experiments. Combining bounds from astrophysical photon spectra with the bounds coming from the mass matrix in the neutrino sector we derive a stringent upper limit for the allowed gravitino mass. This mass limit is in good agreement with the results of direct dark matter searches.

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  • Received 7 June 2011

DOI:https://doi.org/10.1103/PhysRevD.84.055007

© 2011 American Physical Society

Authors & Affiliations

Marco Aurelio Díaz, Sebastián García Sáenz, and Benjamin Koch

  • Departamento de Física, Pontificia Universidad Católica de Chile, Avenida Vicuña Mackenna 4860, Santiago, Chile

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Issue

Vol. 84, Iss. 5 — 1 September 2011

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