Results 21 to 30 of about 28,520 (293)
Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT [PDF]
, 2012 We study the abilities of the Fermi-LAT instrument on board of the Fermi mission to simultaneously constrain the Milky Way dark matter density profile and some dark matter particle properties, as annihilation cross section, mass and branching ratio into ...
Bernal, Nicolas, Palomares-Ruiz, Sergio
core +1 more source
The Milky Way’s halo and subhaloes in self-interacting dark matter [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 ABSTRACT We perform high-resolution simulations of an MW-like galaxy in a self-interacting cold dark matter model with elastic cross-section over mass of $1~\rm cm^2\, g^{-1}$ (SIDM) and compare to a model without self-interactions (CDM).
Victor H Robles +3 more
openaire +4 more sources
Analysis methods for Milky Way dark matter halo detection [PDF]
AIP Conference Proceedings, 2007 We present methods for the analysis of dark matter annihilation in the smooth halo of the Milky Way galaxy. We model the diffuse gamma-ray background using GALPROP, and model the halo using an NFW profile and the gamma-ray spectrum for WIMP pair annihilation.
Aaron Sander +4 more
openaire +1 more source
AN OFF-CENTER DENSITY PEAK IN THE MILKY WAY'S DARK MATTER HALO? [PDF]
The Astrophysical Journal, 2013 12 pages, 11 figures, replaced with version accepted for publication in ...
Kuhlen, M +4 more
openaire +3 more sources
Figure Rotation of IllustrisTNG Halos
The Astrophysical Journal, 2023 We use the TNG50 and TNG50 dark matter (DM)-only simulations from the IllustrisTNG simulation suite to conduct an updated survey of halo figure rotation in the presence of baryons.
Neil Ash, Monica Valluri
doaj +1 more source
DISPERSAL OF TIDAL DEBRIS IN A MILKY-WAY-SIZED DARK MATTER HALO [PDF]
The Astrophysical Journal, 2016 ABSTRACT We simulate the tidal disruption of a collisionless N-body globular star cluster in a total of 300 different orbits selected to have galactocentric radii between 10 and 30 kpc in four dark matter halos: (a) a spherical halo with no subhalos, (b) a spherical halo with subhalos, (c) a realistic halo with no subhalos, and (d) a ...
Ngan W. +5 more
openaire +2 more sources
A mass-dependent density profile for dark matter haloes including the influence of galaxy formation [PDF]
, 2014 We introduce a mass-dependent density profile to describe the distribution of dark matter within galaxies, which takes into account the stellar-to-halo mass dependence of the response of dark matter to baryonic processes.
Aaron A. Dutton +86 more
core +2 more sources
Dark matter annihilation in the Milky Way halo [PDF]
Journal of Physics: Conference Series, 2008 To constrain the particle properties of dark matter using their annihilation products, robust predictions of the annihilation rates are critical. Since the annihilation rate scales as the dark matter density squared, a precise knowledge of the distribution of dark matter is required. Given the popular galactic center contains large uncertainties in the
openaire +1 more source
Dark Matter Substructure and Gamma‐Ray Annihilation in the Milky Way Halo [PDF]
The Astrophysical Journal, 2007 15 pages, 10 figures. ApJ accepted. Movies, images and a version with higher resolution figures are available at http://www.ucolick.org/~diemand/vl/
Diemand, J, Kuhlen, M, Madau, P
openaire +4 more sources
Imprints of flavor anomalies on neutrino oscillations through dark matter halo
Nuclear Physics B, 2023 In this work we study the impact of new physics, stimulated by flavor anomalies, on neutrino oscillations through dense dark matter halo. Inspired by a model where a Majorana dark matter fermion and two new scalar fields contribute to b→sμ+μ− transition ...
Ashutosh Kumar Alok +2 more
doaj +1 more source