Results 11 to 20 of about 565,196 (354)

The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias [PDF]

open access: yesMNRAS, 472, 1088-1105 (2017), 2017
Dark matter halo clustering depends not only on halo mass, but also on other properties such as concentration and shape. This phenomenon is known broadly as assembly bias.
Bosch, Frank C. van den   +8 more
core   +2 more sources

How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering [PDF]

open access: yes, 2018
Clustering of dark matter halos has been shown to depend on halo properties beyond mass such as halo concentration, a phenomenon referred to as halo assembly bias.
Hahn, ChangHoon, Vakili, Mohammadjavad
core   +2 more sources

Evidence for an Intermediate-mass Milky Way from Gaia DR2 Halo Globular Cluster Motions [PDF]

open access: yesAstrophysical Journal, 2018
We estimate the mass of the Milky Way (MW) within 21.1 kpc using the kinematics of halo globular clusters (GCs) determined by Gaia. The second Gaia data release (DR2) contained a catalog of absolute proper motions (PMs) for a set of Galactic GCs and ...
L. Watkins   +4 more
semanticscholar   +1 more source

Novel ultrasonographic Halo Score for giant cell arteritis: assessment of diagnostic accuracy and association with ocular ischaemia

open access: yesAnnals of the Rheumatic Diseases, 2020
Objectives Ultrasound of temporal and axillary arteries may reveal vessel wall inflammation in patients with giant cell arteritis (GCA). We developed a ultrasound scoring system to quantify the extent of vascular inflammation and investigated its ...
Ksm van der Geest   +7 more
semanticscholar   +1 more source

An Accurate Physical Model for Halo Concentrations [PDF]

open access: yesAstrophysical Journal, 2018
The relation between halo mass, M, and concentration, c, is a critical component in our understanding of the structure of dark matter halos. While numerous models for this relation have been proposed, almost none of them attempt to derive the evolution ...
B. Diemer, M. Joyce
semanticscholar   +1 more source

Magnetic field–induced pair density wave state in the cuprate vortex halo [PDF]

open access: yesScience, 2018
Decoding the halo pattern Magnetic fields can cause the formation of vortices in a superconductor. In cuprate superconductors, the vortex cores are surrounded by “halos,” where the density of electronic states exhibits a checkerboard pattern.
S. Edkins   +10 more
semanticscholar   +1 more source

Phases of the Bose–Einstein Condensate Dark Matter Model with Both Two- and Three-Particle Interactions

open access: yesUniverse, 2021
In this paper, we further elaborate on the Bose–Einstein condensate (BEC) dark matter model extended in our previous work [Phys. Rev. D 2020, 102, 083510] by the inclusion of sixth-order (or three-particle) repulsive self-interaction term.
Alexandre M. Gavrilik   +1 more
doaj   +1 more source

Stable clustering, the halo model and non-linear cosmological power spectra [PDF]

open access: yes, 2002
We present the results of a large library of cosmological N-body simulations, using power-law initial spectra.
R. E. Smith   +9 more
semanticscholar   +1 more source

A physical and concise halo model based on the depletion radius [PDF]

open access: yes, 2023
We develop a self-consistent and accurate halo model by partitioning matter according to the depletion radii of haloes. Unlike conventional models that define haloes with the virial radius while relying on a separate exclusion radius or ad-hoc fixes to account for halo exclusion, our model distributes mass across all scales self-consistently and ...
arxiv   +1 more source

Does intraocular straylight predict night driving visual performance? Correlations between straylight levels and contrast sensitivity, halo size, and hazard recognition distance with and without glare

open access: yesFrontiers in Human Neuroscience, 2022
PurposeTo evaluate the relationship between intraocular straylight perception and: (i) contrast sensitivity (CS), (ii) halo size, and (iii) hazard recognition distance, in the presence and absence of glare.Subjects and methodsParticipants were 15 (5 ...
Judith Ungewiss   +8 more
doaj   +1 more source

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