Lyman α emitters gone missing: evidence for late reionization?
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. Th...
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Published: |
Oxford University Press
2015
|
| Subjects: | |
| Online Access: | https://eprints.nottingham.ac.uk/34606/ |
| _version_ | 1848794892740853760 |
|---|---|
| author | Choudhury, Tirthankar Roy Puchwein, Ewald Haehnelt, Martin G. Bolton, James S. |
| author_facet | Choudhury, Tirthankar Roy Puchwein, Ewald Haehnelt, Martin G. Bolton, James S. |
| author_sort | Choudhury, Tirthankar Roy |
| building | Nottingham Research Data Repository |
| collection | Online Access |
| description | 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. |
| first_indexed | 2025-11-14T19:23:25Z |
| format | Article |
| id | nottingham-34606 |
| institution | University of Nottingham Malaysia Campus |
| institution_category | Local University |
| last_indexed | 2025-11-14T19:23:25Z |
| publishDate | 2015 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | nottingham-346062024-08-15T15:17:19Z https://eprints.nottingham.ac.uk/34606/ Lyman α emitters gone missing: evidence for late reionization? Choudhury, Tirthankar Roy Puchwein, Ewald Haehnelt, Martin G. Bolton, James S. 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. Oxford University Press 2015-09-01 Article PeerReviewed Choudhury, Tirthankar Roy, Puchwein, Ewald, Haehnelt, Martin G. and Bolton, James S. (2015) Lyman α emitters gone missing: evidence for late reionization? Monthly Notices of the Royal Astronomical Society, 452 (1). pp. 261-277. ISSN 1365-2966 Intergalactic Medium Cosmology Theory Dark Ages Reionization First Stars Large-scale Structure of the Universe http://mnras.oxfordjournals.org/content/452/1/261 doi:10.1093/mnras/stv1250 doi:10.1093/mnras/stv1250 |
| spellingShingle | Intergalactic Medium Cosmology Theory Dark Ages Reionization First Stars Large-scale Structure of the Universe Choudhury, Tirthankar Roy Puchwein, Ewald Haehnelt, Martin G. Bolton, James S. Lyman α emitters gone missing: evidence for late reionization? |
| title | Lyman α emitters gone missing: evidence for late reionization? |
| title_full | Lyman α emitters gone missing: evidence for late reionization? |
| title_fullStr | Lyman α emitters gone missing: evidence for late reionization? |
| title_full_unstemmed | Lyman α emitters gone missing: evidence for late reionization? |
| title_short | Lyman α emitters gone missing: evidence for late reionization? |
| title_sort | lyman α emitters gone missing: evidence for late reionization? |
| topic | Intergalactic Medium Cosmology Theory Dark Ages Reionization First Stars Large-scale Structure of the Universe |
| url | https://eprints.nottingham.ac.uk/34606/ https://eprints.nottingham.ac.uk/34606/ https://eprints.nottingham.ac.uk/34606/ |