M. Leo
Nonlinear growth of structure in cosmologies with damped matter fluctuations
Leo, M.; Baugh, C.M.; Li, B.; Pascoli, S.
Authors
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
Professor Baojiu Li baojiu.li@durham.ac.uk
Professor
S. Pascoli
Abstract
We investigate the nonlinear evolution of structure in variants of the standard cosmological model which display damped density fluctuations relative to cold dark matter (e.g. in which cold dark matter is replaced by warm or interacting DM). Using N-body simulations, we address the question of how much information is retained from different scales in the initial linear power spectrum following the nonlinear growth of structure. We run a suite of N-body simulations with different initial linear matter power spectra to show that, once the system undergoes nonlinear evolution, the shape of the linear power spectrum at high wavenumbers does not affect the non-linear power spectrum, while it still matters for the halo mass function. Indeed, we find that linear power spectra which differ from one another only at wavenumbers larger than their half-mode wavenumber give rise to (almost) identical nonlinear power spectra at late times, regardless of the fact that they originate from different models with damped fluctuations. On the other hand, the halo mass function is more sensitive to the form of the linear power spectrum. Exploiting this result, we propose a two parameter model of the transfer function in generic damped scenarios, and show that this parametrisation works as well as the standard three parameter models for the scales on which the linear spectrum is relevant.
Citation
Leo, M., Baugh, C., Li, B., & Pascoli, S. (2018). Nonlinear growth of structure in cosmologies with damped matter fluctuations. Journal of Cosmology and Astroparticle Physics, 2018(08), Article 001. https://doi.org/10.1088/1475-7516/2018/08/001
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 16, 2018 |
Online Publication Date | Aug 1, 2018 |
Publication Date | Aug 1, 2018 |
Deposit Date | Sep 24, 2018 |
Publicly Available Date | Aug 1, 2019 |
Journal | Journal of Cosmology and Astroparticle Physics |
Electronic ISSN | 1475-7516 |
Publisher | IOP Publishing |
Peer Reviewed | Peer Reviewed |
Volume | 2018 |
Issue | 08 |
Article Number | 001 |
DOI | https://doi.org/10.1088/1475-7516/2018/08/001 |
Public URL | https://durham-repository.worktribe.com/output/1313705 |
Related Public URLs | https://arxiv.org/abs/1712.02742 |
Files
Accepted Journal Article
(966 Kb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by-nc-nd/4.0/
Copyright Statement
This Accepted Manuscript is available for reuse under a CC BY-NC-ND 3.0 licence after the 12 month embargo period provided that all the terms of the licence are adhered to.
You might also like
Towards an accurate model of small-scale redshift-space distortions in modified gravity
(2022)
Journal Article
Fast full N-body simulations of generic modified gravity: derivative coupling models
(2022)
Journal Article
Halo merger tree comparison: impact on galaxy formation models
(2021)
Journal Article
Modelling emission lines in star-forming galaxies
(2021)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search