Scattering, damping, and acoustic oscillations: Simulating the structure of dark matter halos with relativistic force carriers
We demonstrate that self-interacting dark matter models with interactions mediated by light particles can have significant deviations in the matter power spectrum and detailed structure of galactic halos when compared to a standard cold dark matter scenario. While these deviations can take the form...
Main Authors: | , , , , |
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Other Authors: | , |
Format: | Article |
Language: | English |
Published: |
American Physical Society,
2014-08-25T12:38:26Z.
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Subjects: | |
Online Access: | Get fulltext |