The escape fraction of ionizing photons during the Epoch of Reionization: observability with the Square Kilometre Array. Issue 4 (18th June 2019)

• Record Type: Journal Article
• Authors: Seiler, Jacob; Hutter, Anne; Sinha, Manodeep; Croton, Darren
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 487:Issue 4(2019)
• Page Start: 5739
• Page End: 5752
• Publication Date: 2019-06-18
• Subjects: galaxies: high-redshift -- intergalactic medium -- dark ages, reionization, first stars; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz1663
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: One of the most important parameters in characterizing the Epoch of Reionization, the escape fraction of ionizing photons, f esc, remains unconstrained both observationally and theoretically. With recent work highlighting the impact of galaxy-scale feedback on the instantaneous value of f esc, it is important to develop a model in which reionization is self-consistently coupled to galaxy evolution. In this work, we present such a model and explore how physically motivated functional forms of f esc affect the evolution of ionized hydrogen within the intergalactic medium. Using the 21 cm power spectrum evolution, we investigate the likelihood of observationally distinguishing between a constant f esc and other models that depend upon different forms of galaxy feedback. We find that changing the underlying connection between f esc and galaxy feedback drastically alters the large-scale 21 cm power. The upcoming Square Kilometre Array Low Frequency instrument possesses the sensitivity to differentiate between our models at a fixed optical depth, requiring only 200 h of integration time focused on redshifts z = 7.5–8.5. Generalizing these results to account for a varying optical depth will require multiple 800 h observations spanning redshifts z = 7–10. This presents an exciting opportunity to observationally constrain one of the most elusive parameters during the Epoch of Reionization.