Late-end reionization with ATON-HE: towards constraints from Lyman-α emitters observed with JWST
arxiv(2024)
摘要
We present a new suite of late-end reionization simulations performed with
ATON-HE, a revised version of the GPU-based radiative transfer code ATON that
includes helium. The simulations are able to reproduce the Lyα flux
distribution of the E-XQR-30 sample of QSO absorption spectra at 5 ≲ z
≲ 6.2, and show that a large variety of reionization models are
consistent with these data. We explore a range of variations in source models
and in the early-stage evolution of reionization. Our fiducial reionization
history has a midpoint of reionization at z = 6.5, but we also explore an
`Early' reionization history with a midpoint at z = 7.5 and an `Extremely
Early' reionization history with a midpoint at z = 9.5. Haloes massive enough
to host observed Lyα emitters are highly biased. The fraction of such
haloes embedded in ionized bubbles that are large enough to allow high
Lyα transmission becomes close to unity much before the volume filling
factor of ionized regions. For our fiducial reionization history this happens
at z = 8, probably too late to be consistent with the detection by JWST of
abundant Lyα emission out to z = 11. A reionization history in our
`Early' model or perhaps even our `Extremely Early' model may be required,
suggesting a Thomson scattering optical depth in tension with that reported by
Planck, but consistent with recent suggestions of a significantly higher value.
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