Galaxy Clusters and Dark Matter Properties

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dc.creatorArabadjis, J. S.
dc.creatorBautz, M. W.
dc.date2005-03-07
dc.date.accessioned2026-07-07T02:17:10Z
dc.date.available2026-07-07T02:17:10Z
dc.descriptionLaboratory 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.
dc.descriptionproceedings contribution, "22nd Texas Symposium on Relativistic Astrophysics," Stanford University, 13-17 December 2004; 4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0503146
dc.identifierhttp://arxiv.org/abs/astro-ph/0503146
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9073
dc.subjectAstrophysics
dc.titleGalaxy Clusters and Dark Matter Properties
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