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The influence of metagalactic ultra-violet background fluctuations on the high-redshift Lyα forest

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https://academic.oup.com/mnras/article/491/4/4884/5670635
Original languageEnglish
Pages (from-to)4884-4893
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume491
Issue number4
Early online date9 Dec 2019
DOIs
Publication statusPublished - 1 Feb 2020

Abstract

Under the assumption that galaxies and Quasi-Stellar Objects (QSOs) dominate the metagalactic ultra-violet (UV) background, it is shown that at high redshifts fluctuations in the UV background are dominated by QSO shot noise and have an auto-correlation length of a few to several comoving Mpcs, depending on the bright end of the QSO luminosity function. The correlations create long range spatial coherence in the neutral hydrogen fraction. Using a semi-analytic model, it is demonstrated that the coherence may account for the broad distribution in effective optical depths measured in the Ly forest spectra of background QSOs, for line-of-sight segments of commoving length 50h-1 Mpc at redshifts 5 < z < 6. Capturing the fluctuations in a numerical simulation requires a comoving box size of ~ 1 Gpc, although a box half this size may be adequate if sufficient random realizations of the QSO population are performed.

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