Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3773
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dc.contributor.authorDatta, B-
dc.contributor.authorSivaram, C-
dc.contributor.authorGhosh, S. K-
dc.date.accessioned2008-09-22T15:26:02Z-
dc.date.available2008-09-22T15:26:02Z-
dc.date.issued1985-04-
dc.identifier.citationAstrophysics and Space Science, Vol. 111, No. 2, pp. 413 - 417en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/3773-
dc.description.abstractSeveral independent considerations which rule out the hypothesis that the missing mass in galactic halos is composed of massive neutral fermions such as neutrinos, gravitinos, or photinos are discussed. It is found that the hypothesis does not naturally account for the observational features of such halos as the flat rotation curves and density distributions. The inadequacy of nonprimordial neutrinos to explain the discrepant mass is shown. It is concluded that neutrinos, gravitinos, and photinos are unsatisfactory candidates for the missing matter in galactic halos.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/k125240203342064/en
dc.subjectBig Bang Cosmologyen
dc.subjectFermionsen
dc.subjectGalactic Clustersen
dc.subjectGalactic Evolutionen
dc.subjectMissing Mass (Astrophysics)en
dc.subjectNeutral Particlesen
dc.subjectGravitinosen
dc.subjectHalosen
dc.subjectNeutrinosen
dc.subjectParticle Massen
dc.subjectParticle Theoryen
dc.titleNeutral fermions as the missing mass matter in galactic halosen
dc.typeArticleen
Appears in Collections:IIAP Publications

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