2006/02/28 by J. Hall, Jeter Hall, Paolo Gondolo · 2 citations
Physics and Astronomy · #Annihilation #Astronomy #Astrophysics #Center (category theory) #Center of mass (relativistic) #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Energy–momentum relation #Galactic Center #Galaxy #Milky Way #Neutralino #Particle physics #Particle physics theoretical and experimental studies #Physics #Scalar field dark matter #WIMP #Weakly interacting massive particles #astro-ph
paper · pdf · doi:10.1103/physrevd.74.063511
published as Phys.Rev. D74 (2006) 063511 · replaced with accepted version, improved presentation, some figures corrected, results unchanged
arxiv created 2006/08/18 · openalex publication_date 2006/09/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Dark matter annihilation has been proposed to explain the TeV gamma rays observed from the Galactic Center. We study constraints on this hypothesis coming from the mass profile around the Galactic Center measured by observing stellar dynamics. We show that for several proposed WIMP candidates, the constraints on the dark matter density profile from measurements of mass by infrared observations are comparable to the constraints from the measurements of the TeV source extension.