Neutrinos galactic dark matter and flat rotation curves

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4274

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2009-01-22T16:30:41Z	-
dc.date.available	2009-01-22T16:30:41Z	-
dc.date.issued	1987	-
dc.identifier.citation	Acta Astronomica, Vol. 37, No. 3, pp. 261 - 269	en
dc.identifier.issn	0001-5237	-
dc.identifier.uri	http://hdl.handle.net/2248/4274	-
dc.description.abstract	Degenerate or partially degenerate density distributions of neutrinos do not give rise to flat rotation curves. If the galactic dark matter chiefly consists of neutrinos they would have to be isothermal. Such a halo of thermal neutrinos would, however, dissipate on time scales substantially shorter than typical galaxy ages. Comparison with other forms of dark matter is also made and sensitivity to inclusion of baryons in the core is also studied.	en
dc.language.iso	en	en
dc.publisher	Copernicus Foundation for Polish Astronomy	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987AcA....37..261S	en
dc.subject	Inflationary Universe Models	en
dc.subject	Clustering of Quasar Redshifts	en
dc.title	Neutrinos galactic dark matter and flat rotation curves	en
dc.type	Article	en
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