Results 91 to 100 of about 917,117 (194)

A superfluid dark matter cosmic string wake

open access: yesEuropean Physical Journal C: Particles and Fields
We study the effects of superfluid dark matter on the structure of a cosmic string wake, considering both the effects of regular and quantum pressure terms. We consider the total fluid to consist of a combination of baryons and dark matter. Hence, we are
Aline Favero, Robert Brandenberger
doaj   +1 more source

GeV-scale dark matter: production at the Main Injector

open access: yes, 2014
Assuming that dark matter particles interact with quarks via a GeV-scale mediator, we study dark matter production in fixed target collisions. The ensuing signal in a neutrino near detector consists of neutral-current events with an energy distribution ...
Dobrescu, Bogdan A., Frugiuele, Claudia
core   +1 more source

Polarized equatorial emission and hot spots around black holes with a dark matter halo

open access: yesEuropean Physical Journal C: Particles and Fields
We study linear polarization of the accretion disks around black holes with a dark matter halo. The interaction of the black hole with the dark matter is modeled by considering an exact solution to the Einstein equations which describe a superposition of
Tsanimir Angelov   +4 more
doaj   +1 more source

Distribution of Dark Matter in Galaxies, In Search of the Dark Matter Particle

open access: yesIOSR Journal of Applied Physics, 2014
A new theory called, the Dark Matter Flow Theory based on fluid mechanics concepts, has been given for the first time to derive the density of the dark matter and its distribution inside galaxies and beyond. Although the results are chocking, however they exhibit a high congruence with the measured observations of the velocity rotation curves of ...
openaire   +1 more source

The Impact of Dark Matter on Gravitational Wave Detection by Space-Based Interferometers

open access: yesUniverse
The existence of dark matter is supported by multiple astrophysical observations, yet its particle nature remains unknown. The development of gravitational wave astronomy, especially with future space-based detectors such as LISA, provides new ...
Yuezhe Chen   +4 more
doaj   +1 more source

Determination of dark matter distribution in Ursa Major III and constraints on dark matter annihilation*

open access: yesChinese Physics C
Abstract The recently discovered satellite dwarf galaxy Ursa Major III provides a promising opportunity to explore the signatures resulting from dark matter (DM) annihilation owing to its proximity and large J-factor. Given the absence of an excess of γ-ray signatures originating from Ursa Major III, observations of γ-rays, such as those
Zhao, Yi   +3 more
openaire   +2 more sources

The Distribution of Dark Matter in Spirals [PDF]

open access: yesEAS Publications Series, 2006
In the past years a wealth of observations allowed to unravel the structural properties of the Dark Matter Halos around spirals. First, their rotation curves follow an Universal profile (URC) that can be described in terms of an exponential thin stellar disk and a dark halo with a constant density core, whose relative importance increases with galaxy ...
openaire   +3 more sources

The distribution of dark matter in galaxies [PDF]

open access: yesThe Astronomy and Astrophysics Review, 2019
60 pages, 28 Figures ~220 refs. Invited review for The Astronomy and Astrophysics Review.
openaire   +2 more sources

Microgalaxies in LCDM

open access: yesThe Astrophysical Journal
A fundamental prediction of the Lambda cold dark matter cosmology is the centrally divergent cuspy density profile of dark matter haloes. Density cusps render cold dark matter haloes resilient to tides, and protect dwarf galaxies embedded in them from ...
Raphaël Errani   +4 more
doaj   +1 more source

Dark Matter Structures in the Universe: Prospects for Optical Astronomy in the Next Decade

open access: yes, 2009
The Cold Dark Matter theory of gravitationally-driven hierarchical structure formation has earned its status as a paradigm by explaining the distribution of matter over large spans of cosmic distance and time. However, its central tenet, that most of the
Auger, M.   +15 more
core   +1 more source

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