Results 11 to 20 of about 120,847 (208)

Spatial Distribution of Intracluster Light versus Dark Matter in Horizon Run 5

open access: yesThe Astrophysical Journal
One intriguing approach for studying the dynamical evolution of galaxy clusters is to compare the spatial distributions among various components such as dark matter, member galaxies, gas, and intracluster light (ICL).
Jaewon Yoo   +13 more
doaj   +2 more sources

On the Spatial Distribution of Dark Matter Halos

open access: yesThe Astrophysical Journal, 1998
We study the spatial distribution of dark matter halos in the Universe in terms of their number density contrast, related to the underlying dark matter fluctuation via a non-local and non-linear bias random field. The description of the matter dynamics is simplified by adopting the `truncated' Zel'dovich approximation to obtain both analytical results ...
CATELAN P.   +2 more
openaire   +4 more sources

Radial dependence of the dark matter distribution in M33 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
The stellar and gaseous mass distributions, as well as the extended rotation curve in the nearby galaxy M33 are used to derive the radial distribution of dark matter density in the halo and to test cosmological models of galaxy formation and evolution. Two methods are examined to constrain dark mass density profiles.
Lopez Fune E., Salucci P., Corbelli E.
openaire   +5 more sources

The distribution of dark matter in galaxies [PDF]

open access: yesThe Astronomy and Astrophysics Review, 2019
60 pages, 28 Figures ~220 refs. Invited review for The Astronomy and Astrophysics Review.
Salucci, P.
openaire   +3 more sources

Distribution of phantom dark matter in dwarf spheroidals [PDF]

open access: yesAstronomy & Astrophysics, 2020
We derive the distribution of the phantom dark matter in the eight classical dwarf galaxies surrounding the Milky Way, under the assumption that modified Newtonian dynamics (MOND) is the correct theory of gravity. According to their observed shape, we model the dwarfs as axisymmetric systems, rather than spherical systems, as usually assumed.
Alistair O. Hodson   +2 more
openaire   +3 more sources

An excursion set model for the distribution of dark matter and dark matter haloes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1998
A model of the gravitationally evolved dark matter distribution, in the Eulerian space, is developed. It is a simple extension of the excursion set model that is commonly used to estimate the mass function of collapsed dark matter haloes. In addition to describing the evolution of the dark matter itself, the model allows one to describe the evolution ...
Ravi Sheth
openaire   +3 more sources

The Distribution of Dark Matter in Spirals [PDF]

open access: yesEAS Publications Series, 2006
In the past years a wealth of observations allowed to unravel the structural properties of the Dark Matter Halos around spirals. First, their rotation curves follow an Universal profile (URC) that can be described in terms of an exponential thin stellar disk and a dark halo with a constant density core, whose relative importance increases with galaxy ...
P. Salucci, Salucci, Paolo
openaire   +4 more sources

The distribution of inelastic dark matter in the Sun [PDF]

open access: yesEuropean Physical Journal C: Particles and Fields, 2018
If dark matter is composed of new particles, these may become captured after scattering with nuclei in the Sun, thermalize through additional scattering, and finally annihilate into neutrinos that can be detected on Earth.
Mattias Blennow   +2 more
doaj   +2 more sources

Mixed dark matter from axino distribution [PDF]

open access: yesPhysical Review D, 1994
Figures added, references fixed. Version accepted for publication on Phys. Rev. D. LaTeX.
Bonometto, S. A.   +2 more
openaire   +3 more sources

How does dark matter affect compact star properties and high density constraints of strongly interacting matter [PDF]

open access: yesEPJ Web of Conferences, 2022
We study the impact of asymmetric bosonic dark matter on neutron star properties, including possible changes of tidal deformability, maximum mass, radius, and matter distribution inside the star.
Sagun Violetta   +4 more
doaj   +1 more source

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