Cowsik, R. ; Ratnam, Charu ; Bhattacharjee, P. (1996) Dispersion velocity of galactic dark matter particles Physical Review Letters, 76 (21). pp. 3886-3889. ISSN 0031-9007
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Official URL: http://prl.aps.org/abstract/PRL/v76/i21/p3886_1
Related URL: http://dx.doi.org/10.1103/PhysRevLett.76.3886
Abstract
The self-consistent spatial distribution of particles of galactic dark matter is derived including their own gravitational potential, as also of that of the visible matter of the Galaxy. In order to reproduce the observed rotation curve of the Galaxy the value of the dispersion velocity of the dark matter particles, <v2>½DM should be ~600 km s-1 or larger.
Item Type: | Article |
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Source: | Copyright of this article belongs to American Physical Society. |
ID Code: | 20704 |
Deposited On: | 20 Nov 2010 13:42 |
Last Modified: | 17 May 2016 04:58 |
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