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Evidence of patchy hydrogen reionization from an extreme Ly$\alpha$ trough below redshift six

, , , , , and . (2014)cite arxiv:1407.4850Comment: 19 pages, 20 figures, submitted to MNRAS, comments welcome.

Abstract

We report the discovery of an extremely long ($\sim$110 Mpc/$h$) and dark ($\tau_eff 7$) Ly$\alpha$ trough extending down to $z 5.5$ towards the $z_em 6.0$ quasar ULAS J0148+0600. We use these new data in combination with Ly$\alpha$ forest measurements from 42 quasars at $4.5 z_em 6.4$ to conduct an updated analysis of the line-of-sight variance in the intergalactic Ly$\alpha$ opacity over $4 z 6$. We find that the scatter in transmission among lines of sight near $z 6$ significantly exceeds theoretical expectations for either a uniform ultraviolet background (UVB) or simple fluctuating UVB models in which the mean free path to ionizing photons is spatially invariant. The data, particularly near $z 5.6$-5.8, instead require fluctuations in the volume-weighted hydrogen neutral fraction that are a factor three or more beyond those expected from density variations alone. We argue that these fluctuations are most likely driven by large-scale variations in the mean free path, consistent with expectations for the final stages of inhomogeneous hydrogen reionization. Even by $z 5.6$, however, a large fraction of the data is consistent with a uniform UVB, and by $z 5$ the data are fully consistent with opacity fluctuations arising solely from the density field. This suggests that while reionization may be ongoing at $z 6$, it has fully completed by $z \sim 5$.

Description

[1407.4850] Evidence of patchy hydrogen reionization from an extreme Ly$\alpha$ trough below redshift six

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