File(s) not publicly available
The physics of Reionization: processes relevant for SKA observations
The local intensity of the 21 cm signal emitted during the Epoch of Reionization that will be mapped by the SKA is modulated by the amount of neutral hydrogen. Consequently, understanding the process of reionization of the intergalactic medium (IGM) is crucial for predicting and interpreting the upcoming observations. After presenting the basic physics and most meaningful quantities pertaining to the process of reionization, we will review recent progress in our understanding of the production and escape of ionizing photons in primordial galaxies and of their absorption in the IGM especially in so-called minihalos and Lyman Limit Systems.
History
Publication status
- Published
Publisher
Dolman ScottVolume
2Page range
1683-1692Book title
Advancing astrophysics with the Square Kilometre ArrayPlace of publication
Thatcham, UKISBN
9781909204713Department affiliated with
- Physics and Astronomy Publications
Notes
Paper given at the conference "Advancing Astrophysics with the Square Kilometre Array" (9-13 June, 2014 Giardini Naxos, Italy)Full text available
- No
Peer reviewed?
- Yes
Editors
SKA OrganisationLegacy Posted Date
2017-08-04First Open Access (FOA) Date
2017-08-02First Compliant Deposit (FCD) Date
2017-08-02Usage metrics
Categories
No categories selectedKeywords
Licence
Exports
RefWorks
BibTeX
Ref. manager
Endnote
DataCite
NLM
DC