Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2869
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dc.contributor.authorCowsik, R-
dc.contributor.authorRatnam, C-
dc.contributor.authorBhattacharjee, P-
dc.date.accessioned2008-07-24T05:15:07Z-
dc.date.available2008-07-24T05:15:07Z-
dc.date.issued1996-05-
dc.identifier.citationPhysical Review Letters, Vol. 76, No. 21, pp. 3886 - 3889en
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/2248/2869-
dc.description.abstractThe 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.extent128070 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRL/v76/p3886en
dc.subjectDispersion velocityen
dc.subjectGalactic dark matteren
dc.subjectRotation curveen
dc.titleDispersion Velocity of Galactic Dark Matter Particlesen
dc.typeArticleen
Appears in Collections:IIAP Publications

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