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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| Drugi avtorji: | |
| Format: | Article |
| Jezik: | English |
| Izdano: |
American Physical Society
2014
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| Online dostop: | http://hdl.handle.net/1721.1/89001 https://orcid.org/0000-0001-8593-7692 |