UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

The causal effect of environment on halo mass and concentration

Cadiou, C; Pontzen, A; Peiris, HV; Lucie-Smith, L; (2021) The causal effect of environment on halo mass and concentration. Monthly Notices of the Royal Astronomical Society , 508 (1) pp. 1189-1194. 10.1093/mnras/stab2650. Green open access

[thumbnail of Cadiou_stab2650_VoR.pdf]
Preview
Text
Cadiou_stab2650_VoR.pdf - Published Version

Download (1MB) | Preview

Abstract

Understanding the impact of environment on the formation and evolution of dark matter haloes and galaxies is a crucial open problem. Studying statistical correlations in large simulated populations sheds some light on these impacts, but the causal effect of an environment on individual objects is harder to pinpoint. Addressing this, we present a new method for resimulating a single dark matter halo in multiple large-scale environments. In the initial conditions, we ‘splice’ (i.e. insert) the Lagrangian region of a halo into different Gaussian random fields, while enforcing consistency with the statistical properties of Lambda cold dark matter. Applying this technique, we demonstrate that the mass of haloes is primarily determined by the density structure inside their Lagrangian patches, while the haloes’ concentration is more strongly affected by environment. The splicing approach will also allow us to study, for example, the impact of the cosmic web on accretion processes and galaxy quenching.

Type: Article
Title: The causal effect of environment on halo mass and concentration
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stab2650
Publisher version: http://dx.doi.org/10.1093/mnras/stab2650
Language: English
Additional information: © The Author(s) 2021. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
Keywords: methods: numerical, galaxies: formation, galaxies: haloes, dark matter
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10134974
Downloads since deposit
Loading...
33Downloads
Download activity - last month
Loading...
Download activity - last 12 months
Loading...
Downloads by country - last 12 months
Loading...

Archive Staff Only

View Item View Item