4.7 Article

The effect of inhomogeneous reionization on the Lyman α forest power spectrum at redshift z > 4: implications for thermal parameter recovery

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 509, Issue 4, Pages 6119-+

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab3416

Keywords

methods: numerical; intergalactic medium; quasars: absorption lines; large-scale structure of Universe

Funding

  1. BEIS capital funding via STFC capital grants [ST/P002307/1, ST/R002452/1, ST/P002293/1, ST/R002371/1]
  2. STFC operations grant [ST/R00689X/1, ST/R000832/1]
  3. Durham University
  4. STFC consolidated grant [ST/T000171/1]
  5. Kavli Foundation
  6. UKRI STFC [ST/N000927/1, ST/S000623/1]
  7. Department of Atomic Energy, Government of India [RTI 4002]
  8. Max-Planck-Gesellschaft through a Max Planck Partner Group
  9. European Union [885990]
  10. Marie Curie Actions (MSCA) [885990] Funding Source: Marie Curie Actions (MSCA)
  11. STFC [ST/T000171/1] Funding Source: UKRI

Ask authors/readers for more resources

Using a hybrid hydrodynamical and radiative transfer simulation, we modeled the effect of inhomogeneous reionization on the Lyman alpha forest transmitted flux power spectrum. We found that inhomogeneous reionization can suppress or enhance the power spectrum, highlighting the importance of considering this effect in future high precision measurements.
We use the Sherwood-Relics suite of hybrid hydrodynamical and radiative transfer simulations to model the effect of inhomogeneous reionization on the 1D power spectrum of the Lyman alpha (Ly alpha) forest transmitted flux at redshifts 4.2 <= z <= 5. Relative to models that assume a homogeneous ultraviolet background, reionization suppresses the power spectrum at small scales, k similar to 0.1 km(-1) s, by similar to 10 per cent because of spatial variations in the thermal broadening kernel and the divergent peculiar velocity field associated with overpressurized intergalactic gas. On larger scales, k < 0.03 km(-1) s, the power spectrum is instead enhanced by 10-50 per cent by large-scale spatial variations in the neutral hydrogen fraction. The effect of inhomogeneous reionization must therefore be accounted for in analyses of forthcoming high precision measurements. We provide a correction for the Ly alpha forest power spectrum at 4.1 <= z <= 5.4 that can be easily applied within other parameter inference frameworks using similar reionization models. We perform a Bayesian analysis of mock data to assess the extent of systematic biases that may arise in measurements of the intergalactic medium if ignoring this correction. At the scales probed by current high-resolution Ly alpha forest data at z > 4, 0.006 <= k <= 0.2 km(-1) s, we find inhomogeneous reionization does not introduce any significant bias in thermal parameter recovery for the current measurement uncertainties of similar to 10 per cent. However, for 5 per cent uncertainties, similar to 1 sigma shifts between the estimated and true parameters occur.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available