Results 131 to 140 of about 1,359 (236)

Is the dark-matter halo spin a predictor of galaxy spin and size? [PDF]

open access: bronze, 2019
Fangzhou Jiang   +10 more
openalex   +1 more source

COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions

open access: yesThe Astrophysical Journal
We present eight cosmological dark matter (DM)-only zoom-in simulations of a Milky Way–like system that include suppression of the linear matter power spectrum P ( k ), and/or velocity-dependent DM self-interactions, as the third installment of the ...
Ethan O. Nadler   +5 more
doaj   +1 more source

The “Little Dark Dot”: Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?

open access: yesThe Astrophysical Journal
Previous studies, based on precise modeling of a gravitationally lensing image, have identified what may be an extremely compact, dark perturber in the well-known lensing system SDSS J0946+1006 (the “Jackpot”).
Shubo Li   +15 more
doaj   +1 more source

The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z ~ 1

open access: green, 2004
Charlie Conroy   +8 more
openalex   +1 more source

Relation between the Local Width and Linear Halo Mass Density of Cosmic Filaments

open access: yesThe Astrophysical Journal
Large-scale cosmic filaments may have played an important role in shaping the properties of galaxies. Meanwhile, cosmic filaments are believed to harbor a substantial portion of the missing baryons at redshift z < 2.
Weishan Zhu   +4 more
doaj   +1 more source

The Tidal Torque Theory Revisited. I. Protohalo Angular Momentum

open access: yesThe Astrophysical Journal
In tidal torque theory, the angular momentum (AM) of dark matter halos arises from the tidal torque suffered by aspherical collapsing patches due to surrounding mass fluctuations.
Eduard Salvador-Solé, Alberto Manrique
doaj   +1 more source

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