Non-zero rest mass neutrinos and the cosmological constant

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4378

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2009-03-05T11:21:03Z	-
dc.date.available	2009-03-05T11:21:03Z	-
dc.date.issued	1985-11	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 116, No. 1, pp. 39 - 42	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/4378	-
dc.description.abstract	Recently it was pointed out that a non-zero cosmological constant can play a role in the formation of neutrino halos only in the case of neutrinos of very low rest mass (mν ≤ 0.1 eV). However, phase-space considerations would require mν > 50 eV if neutrinos dominate the missing mass in halos of large spiral galaxies and moreover mν > 200 eV is implied in the case of dwarf spheroidals. These larger neutrino masses would be in conflict with observed constraints on the age of the Universe unless a cosmological constant is invoked.	en
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publisher	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1985Ap%26SS.116...39S	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00649271	en
dc.subject	Computational Astrophysics	en
dc.subject	Constants	en
dc.subject	Cosmology	en
dc.subject	Neutrinos	en
dc.subject	Universe	en
dc.subject	Dwarf Galaxies	en
dc.subject	Missing Mass (Astrophysics)	en
dc.subject	Spiral Galaxies	en
dc.title	Non-zero rest mass neutrinos and the cosmological constant	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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