| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1835475 | Nuclear and Particle Physics Proceedings | 2015 | 8 Pages |
Abstract
Dark matter halos are predicted to be non-spherical by N-body simulations. Using data from the large N-body cosmological simulation Bolshoi, we quantify the systematic uncertainties due to halo asphericity on the determination of local dark matter density and the J factors for dark matter annihilations and decay from the galactic center.
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Physical Sciences and Engineering
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Nuclear and High Energy Physics
