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 ,...
Príomhchruthaitheoirí: | , , |
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Formáid: | Alt |
Teanga: | English |
Foilsithe / Cruthaithe: |
IOP Publishing
2023-01-01
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Sraith: | The Astrophysical Journal |
Ábhair: | |
Rochtain ar líne: | https://doi.org/10.3847/1538-4357/acc73e |