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Les Houches Lectures on Indirect Detection of Dark Matter
SciPost Physics Lecture Notes, 2022 These lectures, presented at the 2021 Les Houches Summer School on Dark Matter, provide an introduction to key methods and tools of indirect dark matter searches, as well as a status report on the field circa summer 2021.
Tracy R. Slatyer
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Astrophysical uncertainties on the local dark matter distribution and direct detection experiments [PDF]
, 2017 The differential event rate in weakly interacting massive particle (WIMP) direct detection experiments depends on the local dark matter density and velocity distribution.
A. Green
semanticscholar +1 more source
DISTRIBUTION FUNCTION OF DARK MATTER WITH CONSTANT ANISOTROPY [PDF]
International Journal of Modern Physics D, 2008 N-body simulations of dark matter halos show that the density is cusped near the center of the halo. The density profile behaves as r–γ in the inner parts, where γ ≃ 1 for the NFW model and γ ≃ 1.5 for the Moore model, but in the outer parts the two models agree with each other in the asymptotic behavior of the density profile.
Ma, Ding, He, Ping
openaire +3 more sources
How does dark matter affect compact star properties and high density constraints of strongly interacting matter [PDF]
EPJ 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
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Dark Matter direct detection of classical WIMPs
SciPost Physics Lecture Notes, 2022 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
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Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity [PDF]
, 2016 We present the radial distribution of the dark matter in two massive, X-ray luminous galaxy clusters, Abell~2142 and Abell~2319, and compare it with the quantity predicted as apparent manifestation of the baryonic mass in the context of the "Emergent ...
S. Ettori +4 more
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Baryonic and dark matter distribution in cosmological simulations of spiral galaxies [PDF]
Monthly notices of the Royal Astronomical Society, 2014 We study three cosmological hydrodynamical simulations of Milky Way(MW)-sized haloes including a comparison with the dark matter(DM)-only counterparts. We find one of our simulated galaxies with interesting MW-like features.
P. Mollitor, E. Nezri, R. Teyssier
semanticscholar +1 more source
Baryonic impact on the dark matter distribution in Milky Way-sized galaxies and their satellites [PDF]
, 2015 We study the impact of baryons on the distribution of dark matter in a Milky Way-size halo by comparing a high-resolution, moving-mesh cosmological simulation with its dark matter-only counterpart.
Qirong Zhu +5 more
semanticscholar +1 more source
The Astrophysical Journal Supplement Series, 2023 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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, 2017 Dark matter in galaxies, its abundance, and its distribution remain a subject of long-standing discussion, especially in view of the fact that neither dark matter particles nor dark matter bodies have yet been found.
Khoperskov, A. V. +3 more
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