UV background fluctuations traced by metal ions at
arXiv:1810.07699 · doi:10.1093/mnrasl/sly199
Abstract
Here we investigate how LyC-opaque systems present in the intergalactic medium at can distort the spectral shape of a uniform UV background (UVB) through radiative transfer (RT) effects. With this aim in mind, we perform a multi-frequency RT simulation through a cosmic volume of ~cMpc scale polluted by metals, and self-consistently derive the ions of all the species. The UVB spatial fluctuations are traced by the ratio of He and H column density, , and the ratio of C and Si optical depths, . We find that: (i) spatially fluctuates through over-dense systems () with statistically significant deviations \% in 18\% of the volume ; (ii) same fluctuations in are also present in \% of the enriched domain (only 8\% of the total volume) and derive from a combination of RT induced effects and in-homogeneous metal enrichment, both effective in systems with .
arXiv commentAccepted for pub. in MNRAS after very minor rev
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