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Dark Matter Halos in Numerical Models at Redshifts 0 ≤ z ≤ 9

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Abstract

For the numerical model in the range of redshifts \(0 \leqslant z \leqslant 9\), we examined the properties and evolution of dark matter halos 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.

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Fig. 1.

Notes

  1. The concentration parameter is defined as cvir = Rvir/r0, where r0 is the characteristic radius in the NFW density profile, see (7) below.

  2. http://www.multidark.es

  3. https://www.cosmosim.org

  4. https://www.cosmosim.org

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ACKNOWLEDGMENTS

The authors are grateful to the anonymous reviewer for helpful comments.

The halo catalogs used in the numerical models are obtained from the CosmoSim database.Footnote 4 This database service is provided by the Institute for Astrophysics Potsdam.

Funding

The study was carried out as part of the Lebedev Physical Institute program NNG 41-2020.

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Authors and Affiliations

  1. Institute of Theoretical Physics, University of Warsaw, Warsaw, Poland

    M. Demiański

  2. Department of Astronomy, Williams College, Williamstown, USA

    M. Demiański

  3. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia

    A. Doroshkevich, T. Larchenkova & S. Pilipenko

  4. National Research Center “Kurchatov Institute”, Moscow, Russia

    A. Doroshkevich

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  1. M. Demiański
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  2. A. Doroshkevich
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Correspondence to M. Demiański.

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Translated by M. Chubarova

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Demiański, M., Doroshkevich, A., Larchenkova, T. et al. Dark Matter Halos in Numerical Models at Redshifts 0 ≤ z ≤ 9. Astron. Rep. 67, 1265–1274 (2023). https://doi.org/10.1134/S1063772923120028

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