Till Sawala
Setting the stage: structures from Gaussian random fields
Sawala, Till; Jenkins, Adrian; McAlpine, Stuart; Jasche, Jens; Lavaux, Guilhem; Johansson, Peter H; Frenk, Carlos S
Authors
Professor Adrian Jenkins a.r.jenkins@durham.ac.uk
Professor
Stuart McAlpine
Jens Jasche
Guilhem Lavaux
Peter H Johansson
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Abstract
We study structure formation in a set of cosmological simulations to uncover the scales in the initial density field that gave rise to the formation of present-day structures. Our simulations share a common primordial power spectrum (here Λ cold dark matter, ΛCDM), but the introduction of hierarchical variations of the phase information allows us to systematically study the scales that determine the formation of structure at later times. We consider the variance in z = 0 statistics such as the matter power spectrum and halo mass function. We also define a criterion for the existence of individual haloes across simulations, and determine what scales in the initial density field contain sufficient information for the non-linear formation of unique haloes. We study how the characteristics of individual haloes such as the mass and concentration, as well as the position and velocity, are affected by variations on different scales, and give scaling relations for haloes of different mass. Finally, we use the example of a cluster-mass halo to show how our hierarchical parametrization of the initial density field can be used to create variants of particular objects. With properties such as mass, concentration, kinematics, and substructure of haloes set on distinct and well-determined scales, and its unique ability to introduce variations localized in real space, our method is a powerful tool to study structure formation in cosmological simulations.
Citation
Sawala, T., Jenkins, A., McAlpine, S., Jasche, J., Lavaux, G., Johansson, P. H., & Frenk, C. S. (2021). Setting the stage: structures from Gaussian random fields. Monthly Notices of the Royal Astronomical Society, 501(4), 4759-4776. https://doi.org/10.1093/mnras/staa3568
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 13, 2020 |
Online Publication Date | Jan 16, 2021 |
Publication Date | 2021-03 |
Deposit Date | Jun 29, 2021 |
Publicly Available Date | Jun 29, 2021 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 501 |
Issue | 4 |
Pages | 4759-4776 |
DOI | https://doi.org/10.1093/mnras/staa3568 |
Public URL | https://durham-repository.worktribe.com/output/1240610 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2021 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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