The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud

@article{Nadler2021TheEO,
  title={The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud},
  author={Ethan O. Nadler and Arka Banerjee and Susmita Adhikari and Yao-Yuan Mao and Risa H. Wechsler},
  journal={The Astrophysical Journal Letters},
  year={2021},
  volume={920}
}
  • E. Nadler, Arka Banerjee, +2 authors R. Wechsler
  • Published 24 September 2021
  • Physics
  • The Astrophysical Journal Letters
Given recent developments in our understanding of the Large Magellanic Cloud's (LMC) impact on the Milky Way's (MW) dark matter subhalo population, we compare the signatures of dark matter and baryonic physics on subhalos in MW systems with realistic LMC analogs. In particular, we study the effects of self-interacting dark matter (SIDM), warm dark matter (WDM), and the Galactic disk on the peak maximum circular velocity (V peak) function, radial distribution, and spatial distribution of MW and… Expand
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