Results 21 to 30 of about 120,847 (208)
Dark Matter direct detection of classical WIMPs
One of the highest priorities in particle physics today is the identification of the constituents of dark matter. This manuscript is a supplement to pedagogical lectures given at the 2021 Les Houches Summer School on Dark Matter.
Jodi Cooley
doaj +1 more source
The local dark matter distribution in self-interacting dark matter halos
Abstract We study the effects of dark matter self-interactions on the local dark matter distribution in selected Milky Way-like galaxies in the EAGLE hydrodynamical simulations. The simulations were run with two different self-interacting dark matter models, a constant and velocity-dependent self-interaction cross-section. We find that
Rahimi, Elham +3 more
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We present spectroscopic data for 16,369 stellar targets within and/or toward 38 dwarf spheroidal galaxies and faint star clusters within the Milky Way halo environment.
Matthew G. Walker +7 more
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Handling the uncertainties in the Galactic Dark Matter distribution for particle Dark Matter searches [PDF]
Updated wrt published version, by including results for Burkert and Einasto profiles.
Benito M., Cuoco A., Iocco F.
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Indirect Evidence for Dark Matter Density Spikes around Stellar-mass Black Holes
It has been suggested for a long time that dark matter would form a density spike around a black hole. However, no promising evidence has been observed so far to verify this theoretical suggestion.
Man Ho Chan, Chak Man Lee
doaj +1 more source
A DERIVATION OF (HALF) THE DARK MATTER DISTRIBUTION FUNCTION [PDF]
All dark matter structures appear to follow a set of universalities, such as phase-space density or velocity anisotropy profiles, however, the origin of these universalities remains a mystery. Any equilibrated dark matter structure can be fully described by two functions, namely the radial and the tangential velocity distribution functions (VDF), and ...
Hansen, Steen Harle, Sparre, Martin
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Clumps and streams in the local dark matter distribution [PDF]
In cold dark matter cosmological models, structures form and grow by merging of smaller units. Numerical simulations have shown that such merging is incomplete; the inner cores of halos survive and orbit as "subhalos" within their hosts. Here we report a simulation that resolves such substructure even in the very inner regions of the Galactic halo.
Diemand, J +6 more
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Probing dark matter with resonant dynamics of the Galactic bar
This thesis provides a novel dynamical evidence for dark matter by measuring for the first time the deceleration of the Galactic bar. This spin-down of the bar requires the transfer of energy and angular momentum to dark matter by dynamical friction ...
Chiba, Rimpei
core +1 more source
Imprint of Pressure on Characteristic Dark Matter Profiles: The Case of ESO0140040
We investigate the dark matter distribution in the spiral galaxy ESO0140040, employing the most widely used density profiles: the pseudo-isothermal, exponential sphere, Burkert, Navarro-Frenk-White, Moore and Einasto profiles.
Kuantay Boshkayev +4 more
doaj +1 more source
On the distribution of dark matter in galaxies: Quantum treatments [PDF]
The problem of modeling the distribution of dark matter in galaxies in terms of equilibrium configurations of collisionless self-gravitating quantum particles is considered. We first summarize the pioneering model of a Newtonian self-gravitating Fermi gas in thermodynamic equilibrium developed by Ruffini and Stella (1983), which is shown to be the ...
Argüelles, Carlos R. +3 more
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