The Three Hundred Project: The evolution of galaxy cluster density profiles. Issue 3 (6th December 2018)

• Record Type: Journal Article
• Authors: Mostoghiu, Robert; Knebe, Alexander; Cui, Weiguang; Pearce, Frazer R; Yepes, Gustavo; Power, Chris; Dave, Romeel; Arth, Alexander
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 483:Issue 3(2019)
• Page Start: 3390
• Page End: 3403
• Publication Date: 2018-12-06
• Subjects: dark matter -- cosmology theory; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty3306
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: Recent numerical studies of the dark matter density profiles of massive galaxy clusters ( M halo > 10 15 M⊙ ) show that their median radial mass density profile remains unchanged up to$z$ > 1, displaying a highly self-similar evolution. We verify this by using the data set of theThe Three Hundred project, i.e. 324 cluster-sized haloes as found in full physics hydrodynamical simulations. We track the progenitors of the mass-complete sample of clusters at$z$ = 0, and find that their median shape is already in place by$z$ = 2.5. However, selecting a dynamically relaxed subsample (∼16 per cent of the clusters), we observe a shift of the scale radius rs towards larger values at earlier times. Classifying the whole sample by formation time, this evolution is understood as a result of a two-phase halo mass accretion process. Early-forming clusters – identified as relaxed today – have already entered their slow accretion phase, hence their mass growth occurs mostly at the outskirts. Late-forming clusters – which are still unrelaxed today – are in their fast accretion phase, thus the central region of the clusters is still growing. We conclude that the density profile of galaxy clusters shows a profound self-similarity out to redshifts$z$ ∼ 2.5. This result holds for both gas and total density profiles when including baryonic physics, as reported here for two rather distinct sub-grid models.