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 ,...
Main Authors: | Daneng Yang, Ethan O. Nadler, Hai-Bo Yu |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acc73e |
Similar Items
-
Orientations of Dark Matter Halos in FIRE-2 Milky Way–mass Galaxies
by: Jay Baptista, et al.
Published: (2023-01-01) -
A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties
by: Ethan O. Nadler, et al.
Published: (2023-01-01) -
Cold Dark Matter and Self-interacting Dark Matter Interpretations of the Strong Gravitational Lensing Object JWST-ER1
by: Demao Kong, et al.
Published: (2024-01-01) -
Tilted Dark Halos Are Common and Long-lived, and Can Warp Galactic Disks
by: Jiwon Jesse Han, et al.
Published: (2023-01-01) -
Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
by: Ethan O. Nadler, et al.
Published: (2023-01-01)