Issue |
A&A
Volume 444, Number 1, December II 2005
|
|
---|---|---|
Page(s) | 45 - 50 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361:20053647 | |
Published online | 21 November 2005 |
Simple models for the distribution of dark matter
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK e-mail: [jin;nwe]@ast.cam.ac.uk
Received:
17
June
2005
Accepted:
17
August
2005
We introduce a simple family of models for representing the dark matter in galaxies. The potential and phase space distribution function are all elementary, while the density is cusped. The models are all hypervirial, that is, the virial theorem holds locally, as well as globally. As an application to dark matter studies, we compute some of the properties of γ-ray sources caused by neutralino self-annihilation in dark matter clumps.
Key words: galaxies: kinematics and dynamics / galaxy: halo / cosmology: dark matter / gamma rays: theory
© ESO, 2005
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.