Results 131 to 140 of about 2,655,258 (212)
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
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
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
Comments on 'Modeling Galaxy Halos Using Dark Matter with Pressure' [PDF]
We comment on the calculational mistake in the paper 'Modeling galaxy halos using dark matter with pressure' by Somnath Bharadwaj and Sayan Kar. The authors made a mistake while calculating the metric, which led to an overestimate of the deflection angle
/Taiwan, Natl. Taiwan U. +3 more
core
A forward modeling approach to analyzing galaxy clustering with SimBIG. [PDF]
Hahn C +9 more
europepmc +1 more source
The James Webb Space Telescope prompts a rethink of how galaxies form. [PDF]
Mann A.
europepmc +1 more source
Network of spin-based sensors constrains topological dark matter. [PDF]
Budker D.
europepmc +1 more source
Stellar feedback drives the baryon deficiency in low-mass galaxies. [PDF]
Yu H +10 more
europepmc +1 more source
Overmassive black holes and little red dots naturally form in simulations. [PDF]
Chon S +4 more
europepmc +1 more source
The abundance and radial distribution of faint and ultra-faint dwarfs in galaxy clusters. [PDF]
Sadhu P +5 more
europepmc +1 more source

