Results 51 to 60 of about 8,080,766 (192)
Python code that implements the dark matter halo contraction given in Cautun et al (2020) and the best fitting Milky Way mass profile given the latest Gaia DR2 rotation curve of our ...
Thomas M. Callingham, Marius Cautun
core +1 more source
Joint Modeling of GD-1 and C-19 as Old Streams
DESI observational data for the GD-1 and C-19 streams are compared to stream simulations in an evolving multihalo potential of a Milky Way–like galaxy based on a cosmological Milky Way–like simulation.
Raymond G. Carlberg +41 more
doaj +1 more source
Stellar Bars in Isolated Gas-rich Spiral Galaxies Do Not Slow Down
Elongated bar-like features are ubiquitous in galaxies, occurring at the centers of approximately two-thirds of spiral disks in the nearby Universe. Due to gravitational interactions between the bar and the other components of galaxies, it is expected ...
Angus Beane +8 more
doaj +1 more source
On the phase-space structure of the Milky Way dark-matter halo
4 pages, 5 figures, uses dunk2001_asp.sty, to appear in "The Dynamics, Structure and History of Galaxies: A Workshop in Honour of Prof. Ken Freeman", (eds) G. S. Da Costa & E. M.
Helmi, Amina +2 more
openaire +3 more sources
Observability of γ rays from dark matter neutralino annihilations in the Milky Way halo [PDF]
44 pages, LaTex, eps figures embedded with epsfig and subfigure ...
Bergström, L. +2 more
openaire +2 more sources
Dark matter direct detection experiments require information about the local dark matter speed distribution to produce constraints on dark matter candidates, or infer their properties in the event of a discovery.
Ethan Lilie +16 more
doaj +1 more source
We discuss formation of dark matter (DM) mini-halos around primordial black holes (PBHs) and its implication on DM direct detection experiments, including axion searches.
Mark P. Hertzberg +2 more
doaj +1 more source
In this work, we utilize a new suite of Milky Way–mass halos from the DREAMS Project, simulated with cold dark matter (CDM), to quantify the influence of baryon feedback and intrinsic halo-to-halo variance on dark matter density profiles.
Alex M. Garcia +25 more
doaj +1 more source
Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
We present Symphony, a compilation of 262 cosmological, cold-dark-matter-only zoom-in simulations spanning four decades of host halo mass, from 10 ^11 –10 ^15 M _⊙ .
Ethan O. Nadler +11 more
doaj +1 more source
International audienceA large simulation reveals that most of the detectable signal from dark matter in our Milky Way probably comes from the main, smooth Galactic halo, rather than from small ...
Stéphane Colombi, Colombi, Stéphane
core +1 more source

