Halo Asymmetry in the Modeling of Galaxy Clustering
Conventional studies of galaxy clustering within the framework of halo models typically assume that the density profile of all dark matter halos can be approximated by the Navarro–Frenk–White (NFW) spherically symmetric profile.
Anna Durkalec +2 more
doaj +1 more source
The James Webb Space Telescope prompts a rethink of how galaxies form. [PDF]
Mann A.
europepmc +1 more source
Linking Warm Dark Matter to Merger Tree Histories via Deep Learning Networks
Dark matter (DM) halos form hierarchically in the Universe through a series of merger events. By pairing halo finder and postprocessing codes, merger series in cosmological simulations can be conveniently represented as a graph-like “tree” structure ...
Ilem Leisher +13 more
doaj +1 more source
The Formation of Dark Matter Halos and High-Redshift Galaxies
In the concordance LCDM cosmological model, galaxies form in the centers of dark matter halos and merge with one another following the mergers of their host halos. Thus, we set out to quantify the growth mechanisms of dark matter halos. For this purpose, we analyze several large N-body simulations of the growth of cosmic structure.
openaire +2 more sources
The era of precision cosmology with voids. [PDF]
Contarini S, Verza G, Pisani A.
europepmc +1 more source
The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]
Taylor ED +9 more
europepmc +1 more source
Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. [PDF]
Di Mascolo L +15 more
europepmc +1 more source
Reduced gas accretion onto galaxies due to effects of external giant radio lobes. [PDF]
Qiu Y, Cen R.
europepmc +1 more source
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
Simulations of multi-phase gas in and around galaxies. [PDF]
Gronke M, E Schneider E.
europepmc +1 more source

