Gravothermal collapse of self-interacting dark matter halos as the origin of intermediate mass black holes in Milky Way satellites
Author:
Funder
Icelandic Research Fund
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.107.083010/fulltext
Reference102 articles.
1. Simulations of the formation, evolution and clustering of galaxies and quasars
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5. A METHOD FOR MEASURING (SLOPES OF) THE MASS PROFILES OF DWARF SPHEROIDAL GALAXIES
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1. Varying primordial state fractions in exo- and endothermic SIDM simulations of Milky Way-mass haloes;Monthly Notices of the Royal Astronomical Society;2024-05-13
2. On the late-time evolution of velocity-dependent self-interacting dark matter halos;Journal of Cosmology and Astroparticle Physics;2024-05-01
3. A parametric model for self-interacting dark matter halos;Journal of Cosmology and Astroparticle Physics;2024-02-01
4. Anisotropic strong lensing as a probe of dark matter self-interactions;Monthly Notices of the Royal Astronomical Society;2023-10-12
5. The impact of baryonic potentials on the gravothermal evolution of self-interacting dark matter haloes;Monthly Notices of the Royal Astronomical Society;2023-09-12
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