Abstract
Inhomogeneous reionization enhances the 1D Ly α forest power spectrum on large scales at redshifts z ≥ 4. This is due to coherent fluctuations in the ionized hydrogen fraction that arise from large-scale variations in the post-reionization gas temperature, which fade as the gas cools. It is therefore possible to use these relic fluctuations to constrain inhomogeneous reionization with the power spectrum at wavenumbers log10(k/km−1 s) ≾ −1.5. We use the Sherwood-Relics suite of hybrid radiation hydrodynamical simulations to perform a first analysis of new Ly α forest power spectrum measurements at 4.0 ≤ z ≤ 4.6. These data extend to wavenumbers log10(k/km−1 s) ≃ −3, with a relative uncertainty of 10–20 per cent in each wavenumber bin. Our analysis returns a 2.7σ preference for an enhancement in the Ly α forest power spectrum at large scales, in excess of that expected for a spatially uniform ultraviolet background. This large-scale enhancement could be a signature of inhomogeneous reionization, although the statistical precision of these data is not yet sufficient for obtaining a robust detection of the relic post-reionization fluctuations. We show that future power spectrum measurements with relative uncertainties of ≾ 2.5 per cent should provide unambiguous evidence for an enhancement in the power spectrum on large scales.
Original language | English |
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Pages (from-to) | 1489-1501 |
Number of pages | 13 |
Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
Volume | 521 |
Issue number | 1 |
DOIs | |
Publication status | Published - 1 May 2023 |
Externally published | Yes |
Keywords
- intergalactic medium
- large-scale structure of Universe
- methods: numerical
- quasars: absorption lines