DARK MATTER HALOS IN NUMERICAL MODELS AT REDSHIFTS 0 ≤ z ≤ 9

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For the numerical model in the range of redshifts \(0 \leqslant z \leqslant 9\), we examined the properties and evolution of dark matter haloes using a previously proposed method of compact analysis that allows separating the influence of random and regular factors on the main characteristics of the dark matter halo. In the investigated range of redshifts, a monotonic evolution of the average values of the basic parameters of small halo structures into a central massive object is observed through sequential hierarchical merging. These basic parameters include the circular velocity \( {{{v}}_{c}} \), the parameter \( {{w}_{c}} = {{{v}}_{c}}{\text{/}}r \), and the mass. In the range \(3 \leqslant z \leqslant 9\), the parameters evolve slowly, while in the range \(0 \leqslant z \leqslant 3\), they evolve rapidly. The evolution of the dark matter halos formed before reionization is characterized by a slow change in their average characteristics and the properties of the halo outskirts. The important role of early-formed massive structural elements is emphasized.

作者简介

Marek Demyanskii

Institute of theoretical physics, University of Warsaw; Department of Astronomy, Williams College

编辑信件的主要联系方式.
Email: astrep@pleiadesonline.com
Poland, Warsaw; USA, Williamstown

Andrei Doroshkevich

P.N. Lebedev physical institute of Russian Academy of Sciences; National Research Center “Kurchatov Institute”

Email: astrep@pleiadesonline.com
Russia, Moscow; Russia, Moscow

Tatiana Larchenkova

P.N. Lebedev physical institute of Russian Academy of Sciences

Email: astrep@pleiadesonline.com
Russia, Moscow

Sergey Pilipenko

P.N. Lebedev physical institute of Russian Academy of Sciences

Email: astrep@pleiadesonline.com
Russia, Moscow

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