The Maximal Neutrino Flux from Neutralino Annihilation in the Galactic   Center
  We discuss a robust and fairly model-independent upper bound on the possible neutrino flux produced by neutralino annihilation in the center of our galaxy, and show that its detection with present or future neutrino telescopes is highly improbable. This bound is obtained by relating the neutrino flux to the gamma flux that would be produced in the same annihilation processes, for which measurements do exist. 
J. Orloff (LPC-Clermont)