Possible evidence for a large-scale enhancement in the Lyman-α forest power spectrum at redshift z ≥ 4

Margherita Molaro, Vid Iršič, James S. Bolton, Maggie Lieu, Laura C. Keating, Ewald Puchwein, Martin G. Haehnelt, Matteo Viel

Research output: Contribution to journalArticlepeer-review

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 languageEnglish
Pages (from-to)1489-1501
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society (MNRAS)
Volume521
Issue number1
DOIs
Publication statusPublished - 1 May 2023
Externally publishedYes

Keywords

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

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