The cosmological constant and galaxy formation

Details The cosmological constant and galaxy formation The cosmological constant and galaxy formation

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242..221d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 15, 1990, p. 221-223. Research supported by S

Mathematics

Logic

5

Cosmology, Dark Matter, Galactic Evolution, Relic Radiation, Astronomical Models, Hubble Constant, Mass Distribution

Scientific paper

A restrictive upper bound is derived for the cosmological constant from the requirement that the formation of galaxies in a cold dark matter scenario should be compatible with the present observational limits for possible anisotropies of the microwave background. If the total density parameters Omega (including the vacuum energy) is equal to the critical value (Omega = 1), the contribution Omega (V) of the vacuum energy density, the conservative bound, Omega (V) is found to be less than 0.7.

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