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Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
Philip Mocz, Anastasia Fialkov, Mark Vogelsberger +11
Bose-Einstein Condensate Dark Matter (BECDM; also known as Fuzzy Dark Matter) is motivated by fundamental physics and has recently received significant attention as a serious alter…
First star-forming structures in fuzzy cosmic filaments
Philip Mocz, Anastasia Fialkov, Mark Vogelsberger +10
In hierarchical models of structure formation, the first galaxies form in low-mass dark matter potential wells, probing the behavior of dark matter on kiloparsec (kpc) scales. Even…
Dark matter haloes and subhaloes
Jesús Zavala, Carlos S. Frenk
The development of methods and algorithms to solve the -body problem for classical, collisionless, non-relativistic particles has made it possible to follow the growth and evolu…
The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
Jesús Zavala, Mark R. Lovell, Mark Vogelsberger +1
Milky Way (MW) satellites reside within dark matter (DM) subhalos with a broad distribution of circular velocity profiles. This diversity is enhanced with the inclusion of ultra-fa…
Self-Interacting Dark Matter Subhalos in the Milky Way's Tides
Omid Sameie, Hai-Bo Yu, Laura V. Sales +2
We study evolution of self-interacting dark matter (SIDM) subhalos in the Milky Way (MW) tidal field. The interaction between the subhalos and the MW's tides lead to more diverse d…
Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
John ZuHone, Jesús Zavala, Mark Vogelsberger
The "sloshing" of the cold gas in the cores of relaxed clusters of galaxies is a widespread phenomenon, evidenced by the presence of spiral-shaped "cold fronts" in X-ray observatio…