Results 41 to 50 of about 781,531 (359)
NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes [PDF]
We use similar to 100 cosmological galaxy formation 'zoom-in' simulations using the smoothed particle hydrodynamics code GASOLINE to study the effect of baryonic processes on the mass profiles of cold dark matter haloes.
A. Dutton+9 more
semanticscholar +1 more source
Primordial Black Holes as Dark Matter: Recent Developments [PDF]
Although the dark matter is usually assumed to be made up of some form of elementary particle, primordial black holes (PBHs) could also provide some of it.
B. Carr, Florian Kuhnel
semanticscholar +1 more source
Gravitational waves from dark matter isocurvature [PDF]
The primordial fluctuations on large scales are adiabatic, but on smaller scales this need not be the case. Here we derive the general analytical framework to compute the stochastic gravitational wave background induced by primordial cold dark matter ...
G. Domènech+2 more
semanticscholar +1 more source
New interactions in the dark sector mediated by dark energy [PDF]
Cosmological observations have revealed the existence of a dark matter sector, which is commonly assumed to be made up of one particle species only. However, this sector might be more complicated than we currently believe: there might be more than one ...
Anthony W. Brookfield+4 more
core +2 more sources
Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
In this paper, after reconstructing the redshift evolution of the Hubble function by adopting Gaussian process techniques, we estimate the best-fit parameters for some flat Friedmann cosmological models based on a modified Chaplygin gas interacting with ...
Muhsin Aljaf+2 more
doaj +1 more source
Cold dark matter plus not-so-clumpy dark relics [PDF]
Various particle physics models suggest that, besides the (nearly) cold dark matter that accounts for current observations, additional but sub-dominant dark relics might exist. These could be warm, hot, or even contribute as dark radiation.
R. Diamanti+4 more
semanticscholar +1 more source
The evolution of large-scale structure in a universe dominated by cold dark matter
The results of numerical simulations of nonlinear gravitational clustering in universes dominated by weakly interacting, 'cold' dark matter are presented.
M. Davis+3 more
semanticscholar +1 more source
The mass–concentration–redshift relation of cold and warm dark matter haloes [PDF]
We use a suite of cosmological simulations to study the mass–concentration–redshift relation, c(M, z), of dark matter haloes. Our simulations include standard Λ-cold dark matter (CDM) models, and additional runs with truncated power spectra, consistent ...
A. Ludlow+7 more
semanticscholar +1 more source
Searching for cold dark matter [PDF]
Latex file, 25 pages , 2 figures (available by fax)
openaire +3 more sources
Crater 2: An Extremely Cold Dark Matter Halo [PDF]
We present results from MMT/Hectochelle spectroscopy of 390 red giant candidate stars along the line of sight to the recently discovered Galactic satellite Crater 2. Modeling the joint distribution of stellar positions, velocities, and metallicities as a
N. Caldwell+8 more
semanticscholar +1 more source