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
Effects of P-wave Annihilation on the Angular Power Spectrum of Extragalactic Gamma-rays from Dark Matter Annihilation [PDF]
We present a formalism for estimating the angular power spectrum of extragalactic gamma-rays produced by dark matter annihilating with any general velocity-dependent cross section.
Bhaskar Dutta +4 more
core +3 more sources
Simple models for the distribution of dark matter [PDF]
to appear in A&A, including 4 figures, appendices B&C are only available through ...
An, Jin H., Evans, N. Wyn
openaire +2 more sources
Dark Matter in Disequilibrium: The Local Velocity Distribution from SDSS-Gaia [PDF]
We use the distribution of accreted stars in SDSS-Gaia DR2 to demonstrate that the local dark matter halo may not be in equilibrium and that a non-trivial fraction is in substructure.
L. Necib, M. Lisanti, V. Belokurov
semanticscholar +1 more source
Variational Distributions & Dark matter
By analyzing the main equation of the 8T in universe packet representation the author expends the idea of "dark energy" an additional gravitational trace from a distinct manifold with isomorphic areas of extremum curvature which have different matter ...
openaire +1 more source
The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO [PDF]
The recent detection by Advanced LIGO of gravitational waves (GW) from the merging of a binary black hole system sets new limits on the merging rates of massive primordial black holes (PBH) that could be a significant fraction or even the totality of the
S. Clesse, J. Garc'ia-Bellido
semanticscholar +1 more source
On the dark matter distribution in the Milky Way
The distribution of dark matter in the Milky Way is a crucial input for ongoing studies in cosmology, astrophysics and particle physics. This motivates the effort over the next years to improve our mapping of dark matter, which has indeed become a top ...
F. Iocco, Miguel Pato
semanticscholar +1 more source
Stellar mass map and dark matter distribution in M 31 [PDF]
Aims. Stellar mass distribution in the Andromeda galaxy (M 31) is estimated using optical and near-infrared imaging data. Combining the derived stellar mass model with various kinematical data, properties of the dark matter (DM) halo of the galaxy are ...
A. Tamm +7 more
semanticscholar +1 more source
Experimental identification of non-pointlike dark-matter candidates [PDF]
We show that direct dark matter detection experiments can distinguish between pointlike and non-pointlike dark-matter candidates. The shape of the nuclear recoil energy spectrum from pointlike dark-matter particles, e.g., neutralinos, is determined by ...
A. Anisimov +15 more
core +2 more sources
The metal-poor stellar halo in RAVE-TGAS and its implications for the velocity distribution of dark matter [PDF]
The local velocity distribution of dark matter plays an integral role in interpreting the results from direct detection experiments. We previously showed that metal-poor halo stars serve as excellent tracers of the virialized dark matter velocity ...
J. Herzog-Arbeitman +2 more
semanticscholar +1 more source

