The effect of inhomogeneous reionisation on the Lyman-$\alpha$ forest power spectrum at redshift $z>4$: implications for thermal parameter recovery
Margherita Molaro, Vid Ir\v{s}i\v{c}, James S. Bolton, Laura C., Keating, Ewald Puchwein, Prakash Gaikwad, Martin G. Haehnelt, Girish, Kulkarni, Matteo Viel

TL;DR
This study models how inhomogeneous reionisation affects the Lyman-alpha forest power spectrum at high redshifts, revealing scale-dependent modifications and providing correction methods for future precise measurements.
Contribution
It introduces a correction for the inhomogeneous reionisation effect on the Lyman-alpha forest power spectrum and assesses its impact on thermal parameter estimation.
Findings
Reionisation suppresses small-scale power by ~10%.
Large-scale power is enhanced by 10-50%.
Ignoring reionisation effects can bias thermal measurements at high precision.
Abstract
We use the Sherwood-Relics suite of hybrid hydrodynamical and radiative transfer simulations to model the effect of inhomogeneous reionisation on the 1D power spectrum of the \Lya forest transmitted flux at redshifts . Relative to models that assume a homogeneous UV background, reionisation suppresses the power spectrum at small scales, by per cent because of spatial variations in the thermal broadening kernel and the divergent peculiar velocity field associated with over-pressurised intergalactic gas. On larger scales, , the power spectrum is instead enhanced by -- per cent by large scale spatial variations in the neutral hydrogen fraction. The effect of inhomogeneous reionisation must therefore be accounted for in analyses of forthcoming high precision measurements. We provide a correction for the…
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