Mathematics – Logic
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370l..15s&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 370, March 20, 1991, p. L15-L18.
Mathematics
Logic
38
Astronomical Models, Dark Matter, Red Shift, Correlation, Galactic Clusters, Galactic Evolution, Hubble Constant, Many Body Problem
Scientific paper
Biased cold dark matter scenario in an Einstein-de Sitter universe is critically examined using the cosmological N-body simulations with N = 128-exp 3 particles. The redshift correlation function zeta-s(s) is used to identify the present epoch of the simulation data, rather than the real space correlation function zeta-r(x). It turned out that both procedures predict quite different fluctuation amplitude to be matched with the present universe, implying that the previous results should be carefully interpreted. The fluctuation amplitude which yields a marginally consistent slope of zeta-s(s) in simulation to the observed value predicts an unacceptably large value for the one-dimensional rms velocity dispersion about 1000 km/s. Therefore, to the extent that the observed zeta-s(s) is reliable as a statistical measure of the fair sample of the universe, the conventional Omega = 1 CDM scenario with the primordial scale-invariant, random-Gaussian density field should be ruled out.
Suginohara Tatsushi
Suto Yasushi
No associations
LandOfFree
Redshift-space correlation functions in the cold dark matter scenario does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Redshift-space correlation functions in the cold dark matter scenario, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Redshift-space correlation functions in the cold dark matter scenario will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1602836