Results 111 to 120 of about 1,187,641 (234)
Stellar streams from globular clusters (GCs) offer constraints on the nature of dark matter and have been used to explore the dark matter halo structure and substructure of our Galaxy. Detection of GC streams in other galaxies would broaden this endeavor
Sarah Pearson +7 more
doaj +1 more source
GHASP: an Hα kinematic survey of spiral and irregular galaxies – V. Dark matter distribution in 36 nearby spiral galaxies [PDF]
The results obtained from a study of the mass distribution of 36 spiral galaxies are presented. The galaxies were observed using Fabry-Perot interferometry as part of the GHASP survey.
Spano M +5 more
semanticscholar +1 more source
Dark Matter Signals in the gamma-ray sky
Detection of gamma rays and cosmic rays from the annihilation or decay of dark matter particles is a promising method for identifying dark matter, understanding its intrinsic properties, and mapping its distribution in the universe.
Morselli Aldo
doaj +1 more source
Time-Dependent Models for Dark Matter at the Galactic Center [PDF]
The prospects of indirect detection of dark matter at the galactic center depend sensitively on the mass profile within the inner parsec. We calculate the distribution of dark matter on sub-parsec scales by integrating the time-dependent Fokker-Planck ...
A. S. Eddington +6 more
core +3 more sources
Apoastron shift constraints on dark matter distribution at the Galactic Center [PDF]
The existence of dark matter (DM) at scales of a few parsecs down to $\ensuremath{\simeq}{10}^{\ensuremath{-}5}\text{ }\text{ }\mathrm{pc}$ around the centers of galaxies and, in particular, in the Galactic Center region has been considered in the ...
A. Zakharov +3 more
semanticscholar +1 more source
We present Multi-resolution MAximum-entropy Reconstruction Technique Integrating Analytic Node ( MrMARTIAN ), a new hybrid strong lensing (SL) modeling algorithm.
Sangjun Cha, M. James Jee
doaj +1 more source
Probing multicomponent extension of inert doublet model with a vector dark matter
Although theoretically well-motivated as a minimal consistent dark matter (DM) model, the inert doublet model (IDM) fell short in explaining the existence of DM in the intermediate mass region (100–500 GeV).
Sreemanti Chakraborti +2 more
doaj +1 more source
The evolution of the dark matter distribution at the Galactic center is analyzed, which is caused by the combination of gravitational scattering on Galactic bulge stars and absorption by a supermassive black hole at the center of the bulge.
A. Lightman +7 more
core +2 more sources
Dark matter distribution function from non-extensive statistical mechanics [PDF]
We present an analytical and numerical study of the velocity distribution function of self gravitating collisionless particles, which include dark matter and star clusters. We show that the velocity distribution derived through the Eddington’s formula is
S. Hansen +3 more
semanticscholar +1 more source
Anisotropy of dark matter velocity distribution
Direct detection of dark matter with directional sensitivity has the potential to discriminate the dark matter velocity distribution. Especially, it will be suitable to discriminate isotropic distribution from anisotropic one. Analyzing data produced with Monte-Carlo simulation, required conditions for the discrimination is estimated.
openaire +2 more sources

