Tirthankar Roy Choudhury
Lyman α emitters gone missing: evidence for late reionization?
Choudhury, Tirthankar Roy; Puchwein, Ewald; Haehnelt, Martin G.; Bolton, James S.
Authors
Ewald Puchwein
Martin G. Haehnelt
JAMES BOLTON James.Bolton@nottingham.ac.uk
Professor of Astrophysics
Abstract
We combine high resolution hydrodynamical simulations with an intermediate resolution, dark matter only simulation and an analytical model for the growth of ionized regions to estimate the large scale distribution and redshift evolution of the visibility of Lyα emission in 6<=z<=8 galaxies. The inhomogeneous distribution of neutral hydrogen during the reionization process results in significant fluctuations in the Lyα transmissivity on large scales. The transmissivity depends not only on the ionized fraction of the intergalactic medium by volume and the amplitude of the local ionizing background, but is also rather sensitive to the evolution of the relative velocity shift of the Lyα emission line due to resonant scattering. We reproduce a decline in the space density of Lyα emitting galaxies as rapid as observed with a rather rapidly evolving neutral fraction between z=6-8, and a typical Lyα line velocity offset of 100 km/s redward of systemic at z=6 which decreases toward higher redshift. The new (02/2015) Planck results indicate such a recent end to reionization is no longer disfavoured by constraints from the cosmic microwave background.
Citation
Choudhury, T. R., Puchwein, E., Haehnelt, M. G., & Bolton, J. S. (2015). Lyman α emitters gone missing: evidence for late reionization?. Monthly Notices of the Royal Astronomical Society, 452(1), 261-277. https://doi.org/10.1093/mnras/stv1250
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 1, 2015 |
Online Publication Date | Jul 2, 2015 |
Publication Date | Sep 1, 2015 |
Deposit Date | Jul 4, 2016 |
Publicly Available Date | Jul 4, 2016 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 452 |
Issue | 1 |
Pages | 261-277 |
DOI | https://doi.org/10.1093/mnras/stv1250 |
Keywords | Intergalactic Medium, Cosmology, Theory, Dark Ages, Reionization, First Stars, Large-scale Structure of the Universe |
Public URL | https://nottingham-repository.worktribe.com/output/757880 |
Publisher URL | http://mnras.oxfordjournals.org/content/452/1/261 |
Additional Information | This article has been published in Monthly Notices of the Royal Astronomical Society ©2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society |
Contract Date | Jul 4, 2016 |
Files
261.full.pdf
(18.8 Mb)
PDF
Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
You might also like
Deep learning the intergalactic medium using lyman-alpha forest at 4 ≤ z ≤ 5
(2024)
Journal Article
Downloadable Citations
About Repository@Nottingham
Administrator e-mail: discovery-access-systems@nottingham.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 © 2024
Advanced Search