A Mass Dependent Density Profile from Dwarfs to Clusters

In this paper, we extend the work of Freundlich et al. 2020 who showed how to obtain a Dekel–Zhao density profile with mass dependent shape parameters in the case of galaxies. In the case of Freundlich et al. 2020, the baryonic dependence was obtained using the NIHAO set of simulations. In our case,...

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Main Authors: Antonino Del Popolo, Morgan Le Delliou
Format: Article
Language:English
Published: MDPI AG 2022-05-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/10/3/69
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author Antonino Del Popolo
Morgan Le Delliou
author_facet Antonino Del Popolo
Morgan Le Delliou
author_sort Antonino Del Popolo
collection DOAJ
description In this paper, we extend the work of Freundlich et al. 2020 who showed how to obtain a Dekel–Zhao density profile with mass dependent shape parameters in the case of galaxies. In the case of Freundlich et al. 2020, the baryonic dependence was obtained using the NIHAO set of simulations. In our case, we used simulations based on a model of ours. Following Freundlich et al. 2020, we obtained the dependence from baryon physics of the two shape parameters, obtaining in this way a mass dependent Dekel–Zhao profile describing the dark matter profiles from galaxies to clusters of galaxies. The extension to the Dekel–Zhao mass dependent profile to clusters of galaxies is the main result of the paper. In the paper, we show how the Dekel–Zhao mass dependent profile gives a good description of the density profiles of galaxies, already shown by Freundlich et al. 2020, but also to a set of clusters of galaxies.
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spelling doaj.art-a762650ec6074ddc9a62bf9995fdebcb2023-11-23T16:44:10ZengMDPI AGGalaxies2075-44342022-05-011036910.3390/galaxies10030069A Mass Dependent Density Profile from Dwarfs to ClustersAntonino Del Popolo0Morgan Le Delliou1Dipartimento di Fisica e Astronomia, University Of Catania, Viale Andrea Doria 6, 95125 Catania, ItalyInstitute of Theoretical Physics, School of Physical Science and Technology, Lanzhou University, No. 222, South Tianshui Road, Lanzhou 730000, ChinaIn this paper, we extend the work of Freundlich et al. 2020 who showed how to obtain a Dekel–Zhao density profile with mass dependent shape parameters in the case of galaxies. In the case of Freundlich et al. 2020, the baryonic dependence was obtained using the NIHAO set of simulations. In our case, we used simulations based on a model of ours. Following Freundlich et al. 2020, we obtained the dependence from baryon physics of the two shape parameters, obtaining in this way a mass dependent Dekel–Zhao profile describing the dark matter profiles from galaxies to clusters of galaxies. The extension to the Dekel–Zhao mass dependent profile to clusters of galaxies is the main result of the paper. In the paper, we show how the Dekel–Zhao mass dependent profile gives a good description of the density profiles of galaxies, already shown by Freundlich et al. 2020, but also to a set of clusters of galaxies.https://www.mdpi.com/2075-4434/10/3/69dark mattergalaxy clustersevolution of the universe
spellingShingle Antonino Del Popolo
Morgan Le Delliou
A Mass Dependent Density Profile from Dwarfs to Clusters
Galaxies
dark matter
galaxy clusters
evolution of the universe
title A Mass Dependent Density Profile from Dwarfs to Clusters
title_full A Mass Dependent Density Profile from Dwarfs to Clusters
title_fullStr A Mass Dependent Density Profile from Dwarfs to Clusters
title_full_unstemmed A Mass Dependent Density Profile from Dwarfs to Clusters
title_short A Mass Dependent Density Profile from Dwarfs to Clusters
title_sort mass dependent density profile from dwarfs to clusters
topic dark matter
galaxy clusters
evolution of the universe
url https://www.mdpi.com/2075-4434/10/3/69
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