The two-point correlation function as an indicator of nonlinear cosmological clumping

Details The two-point correlation function as an indicator of nonlinear cosmological clumping The two-point correlation function as an indicator of nonlinear cosmological clumping

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..519m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Sept. 1983, p. 519-523) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Sept.-Oct

Astronomy and Astrophysics

Astronomy

1

Clumps, Correlation, Cosmology, Galactic Evolution, Computerized Simulation, Fourier Transformation, J Integral, Red Shift

Scientific paper

An explicit counterexample shows that the two-point correlation function xi(R) is not a good measure of the nonlinearity of the large-scale clustering process that occurred when structure was developing in the universe. The xi(R) curve derived from a two-dimensional numerical simulation of the adiabatic scenario for the formation of large-scale structure displays no peculiar features, during the strongly nonlinear stage, that might reflect such clumping.

Affiliated with

Also associated with

No associations

Rating

The two-point correlation function as an indicator of nonlinear cosmological clumping 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 The two-point correlation function as an indicator of nonlinear cosmological clumping, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The two-point correlation function as an indicator of nonlinear cosmological clumping will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1195004