Mond, dark matter and the cosmological constant

dc.contributor.author	Sivaram, C
dc.date.accessioned	2008-08-04T10:20:13Z
dc.date.available	2008-08-04T10:20:13Z
dc.date.issued	1994-09
dc.identifier.citation	Astrophysics and Space Science, Vol. 219, No. 1, pp. 135 - 141	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/2980
dc.description.abstract	A possible connection between MOND (Modification of Newtonian Dynamics) proposed as an alternative hypothesis to dark matter in galaxies and clusters and a residual cosmological constant term dominating cosmological dynamics in a Omega = 1 universe is explored.	en
dc.format.extent	3894 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/l2880650x54u2640/	en
dc.subject	Astrodynamics	en
dc.subject	Constants	en
dc.subject	Cosmology	en
dc.subject	Dark Matter	en
dc.subject	Galactic Clusters	en
dc.subject	Galaxies	en
dc.subject	Missing Mass (Astrophysics)	en
dc.subject	Newton Theory	en
dc.subject	Universe	en
dc.subject	Flux Density	en
dc.subject	Galactic Rotation	en
dc.subject	Poisson Equation	en
dc.subject	Spiral Galaxies	en
dc.subject	Stellar Gravitation	en
dc.subject	Vacuum	en
dc.title	Mond, dark matter and the cosmological constant	en
dc.type	Article	en