2000/06/21 by M. Demiański, M. Demianski, А. G. Doroshkevich +2 · 1 citation
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Dark matter #Distribution (mathematics) #Doppler effect #Entropy (arrow of time) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gaussian #Mathematical analysis #Physics #Quantum mechanics #Redshift #Statistical physics #Stellar, planetary, and galactic studies #Structure formation #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2000.03862.x
published as Mon.Not.Roy.Astron.Soc. 318 (2000) 1189 · 17 pages, 6 Fiures, accepted in MNRAS
arxiv created 2000/06/21 · openalex publication_date 2000/11/11 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The main observed properties of Lyα absorbers are investigated on the basis of a theoretical model of formation and evolution of dark matter (DM) structure elements. This model is generally consistent with simulations of absorber formation and with the statistical description of structure evolution based on the Zel'dovich theory. The analysis of redshift variations of comoving linear number density of absorbers was performed in our previous paper. We show that the observed characteristics of the Doppler parameter can be related to the size of DM structure elements that allow us to explain the observed distribution of the Doppler parameter. This distribution is found to be consistent with the Gaussian initial perturbations. The observed characteristics of entropy and column density NH i confirm that the merging of pancakes is the main evolutionary process at redshifts z⩾2. The observed sample of absorbers mainly characterizes the matter distribution within large low-density regions and therefore it is difficult to reconstruct the density field from the distribution of absorbers.