The hierarchical nature of halo formation in the Cold Dark Matter (CDM) model suggests that there should be mass dependent trends in the radial velocity and velocity anisotropy profiles of dark matter haloes, with more massive systems exhibiting the effects of more pronounced infall. We present results from a sample of high resolution cosmological N-body simulations of individual dwarf, galaxy and cluster mass haloes, and demonstrate that such trends with mass are indeed observed.
We use a set of high-resolution cosmological N-body simulations to investigate the inner mass profil...
We present an analysis of the clustering evolution of dark matter in four cold dark matter (CDM) cos...
We discuss the universal relation between density and size of observed dark matter halos that was re...
The hierarchical nature of halo formation in the Cold Dark Matter (COM) model suggests that there sh...
The balance of evidence indicates that individual galaxies and groups or clusters of galaxies are em...
We use N-body simulations to investigate the structure of dark halos in the standard Cold Dark Matte...
N-body simulations predict that cold dark matter (CDM) halo-assembly occurs in two phases: (i) a fas...
In the standard cosmological model a mysterious cold dark matter (CDM) component dominates the forma...
N-body simulations predict that CDM halo-assembly occurs in two phases: a rapid accretion phase domi...
We use the universal mass accretion history recently reported for simulations of halo formation in t...
In this paper, we analyse in detail the mass-accretion histories and structural properties of dark h...
We study the mass, velocity dispersion and anisotropy profiles of Lambda cold dark matter (Lambda CD...
The cold dark matter spectrum on earth is expected to have peaks in velocity space. We obtain estima...
We use large N-body simulations of dissipationless gravitational clustering in cold dark matter (CDM...
We show by means of a high-resolution N-body simulation how the mass assembly histories of galaxy-si...
We use a set of high-resolution cosmological N-body simulations to investigate the inner mass profil...
We present an analysis of the clustering evolution of dark matter in four cold dark matter (CDM) cos...
We discuss the universal relation between density and size of observed dark matter halos that was re...
The hierarchical nature of halo formation in the Cold Dark Matter (COM) model suggests that there sh...
The balance of evidence indicates that individual galaxies and groups or clusters of galaxies are em...
We use N-body simulations to investigate the structure of dark halos in the standard Cold Dark Matte...
N-body simulations predict that cold dark matter (CDM) halo-assembly occurs in two phases: (i) a fas...
In the standard cosmological model a mysterious cold dark matter (CDM) component dominates the forma...
N-body simulations predict that CDM halo-assembly occurs in two phases: a rapid accretion phase domi...
We use the universal mass accretion history recently reported for simulations of halo formation in t...
In this paper, we analyse in detail the mass-accretion histories and structural properties of dark h...
We study the mass, velocity dispersion and anisotropy profiles of Lambda cold dark matter (Lambda CD...
The cold dark matter spectrum on earth is expected to have peaks in velocity space. We obtain estima...
We use large N-body simulations of dissipationless gravitational clustering in cold dark matter (CDM...
We show by means of a high-resolution N-body simulation how the mass assembly histories of galaxy-si...
We use a set of high-resolution cosmological N-body simulations to investigate the inner mass profil...
We present an analysis of the clustering evolution of dark matter in four cold dark matter (CDM) cos...
We discuss the universal relation between density and size of observed dark matter halos that was re...
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