Dispersion Velocity of Galactic Dark Matter Particles

dc.contributor.author	Cowsik, R
dc.contributor.author	Ratnam, C
dc.contributor.author	Bhattacharjee, P
dc.date.accessioned	2008-07-24T05:15:07Z
dc.date.available	2008-07-24T05:15:07Z
dc.date.issued	1996-05
dc.identifier.citation	Physical Review Letters, Vol. 76, No. 21, pp. 3886 - 3889	en
dc.identifier.issn	0031-9007
dc.identifier.uri	http://hdl.handle.net/2248/2869
dc.description.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>1/2DM should be ~600 km s-1 or larger.	en
dc.format.extent	128070 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRL/v76/p3886	en
dc.subject	Dispersion velocity	en
dc.subject	Galactic dark matter	en
dc.subject	Rotation curve	en
dc.title	Dispersion Velocity of Galactic Dark Matter Particles	en
dc.type	Article	en