SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA

Details SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA

1995-05-30

arxiv.org/abs/astro-ph/9505136v1

Astronomy and Astrophysics

Astrophysics

4 pages uuencoded compressed postscript, to appear in the proceedings of the XXXth MORIOND meeting: "Clustering in the Univers

Scientific paper

A double inflationary model provides perturbation spectra with enhanced power at large scales (Broken Scale Invariant perturbations -- BSI), leading to a promising scenario for the formation of cosmic structures. We describe a series of high-resolution PM simulations with a model for the thermodynamic evolution of baryons in which we are capable of identifying 'galaxy' halos with a reasonable mass spectrum and following the genesis of large and super-large scale structures. The power spectra and correlation functions of 'galaxies' are compared with reconstructed power spectra of the CfA catalogue and the correlation functions of the Las Campanas Deep Redshift Survey.

Affiliated with

Also associated with

No associations

Rating

SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA 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 SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-315488