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Preprint | PUBDB-2022-01926 |
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2022
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Please use a persistent id in citations: doi:10.3204/PUBDB-2022-01926
Report No.: DESY-22-072; arXiv:2205.02243
Abstract: Dark matter (DM) with self-interactions is a promising solution for the small-scale problems of the standard cosmological model. Here we perform the first cosmological simulation of frequent DM self-interactions, corresponding to small-angle DM scatterings. The focus of our analysis lies in finding and understanding differences to the traditionally assumed rare DM (large-angle) self scatterings. For this purpose, we compute the distribution of DM densities, the matter power spectrum, the two-point correlation function and the halo and subhalo mass functions. Furthermore, we investigate the density profiles of the DM haloes and their shapes. We find that overall large-angle and small-angle scatterings behave fairly similarly with a few exceptions. In particular, the number of satellites is considerably suppressed for frequent compared to rare self-interactions with the same cross-section. Overall we observe that while differences between the two cases may be difficult to establish using a single measure, the degeneracy may be broken through a combination of multiple ones. For instance, the combination of satellite counts with halo density or shape profiles could allow discriminating between rare and frequent self-interactions. As a by-product of our analysis, we provide - for the first time - upper limits on the cross-section for frequent self-interactions.
Keyword(s): dark matter, density ; scattering, small-angle ; dark matter, halo ; matter, power spectrum ; dark matter, scattering ; halo, density ; satellite ; wide-angle ; correlation function ; suppression ; cosmological model
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Journal Article
Cosmological simulations with rare and frequent dark matter self-interactions
Monthly notices of the Royal Astronomical Society 516(2), 1923 - 1940 (2022) [10.1093/mnras/stac2207]
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