Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way
We perform a high-resolution cosmological zoom-in simulation of a Milky Way (MW)–like system, which includes a realistic Large Magellanic Cloud analog, using a large differential elastic dark matter self-interaction cross section that reaches ≈100 cm ^2 g ^−1 at relative velocities of ≈10 km s ^−1 ,...
| Váldodahkkit: | , , |
|---|---|
| Materiálatiipa: | Artihkal |
| Giella: | English |
| Almmustuhtton: |
IOP Publishing
2023-01-01
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| Ráidu: | The Astrophysical Journal |
| Fáttát: | |
| Liŋkkat: | https://doi.org/10.3847/1538-4357/acc73e |