Galaxy Clusters and Dark Matter Properties
arXiv:astro-ph/0503146
Abstract
Laboratory experiments, large-scale computer simulations and observational cosmology have begun to make progress in the campaign to identify the particle responsible for gravitationally-inferred dark matter. In this contribution we discuss the dark matter density profiles in the cores of nearby galaxy clusters and estimate the gamma-ray flux expected for MSSM dark matter over a range of neutralino masses.
proceedings contribution, "22nd Texas Symposium on Relativistic Astrophysics," Stanford University, 13-17 December 2004; 4 pages, 5 figures