4.7 Article

Studying the Lyman α optical depth fluctuations at z ∼ 5.5 using fast semi-numerical methods

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 501, Issue 4, Pages 5782-5796

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab045

Keywords

galaxies: high-redshift; intergalactic medium; quasars: absorption lines; dark ages, reionization, first stars

Funding

  1. Department of Atomic Energy, Government of India [12-RD-TFR-5.02-0700]
  2. ICTP
  3. ICTP, Trieste
  4. Ramanujan Fellowship - Department of Science and Technology, Government of India
  5. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program [669253]

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A computationally efficient method is proposed in this study to simulate Lyman alpha absorption optical depth in the presence of neutral hydrogen "islands" leftover from reionization at redshifts between 5 and 6. By analyzing large-scale fluctuations in optical depth, it is confirmed at greater than or similar to 2 sigma confidence that reionization is not complete before around 5.6, with a possibility of completion as late as around 5.2.
We present a computationally efficient and fast semi-numerical technique for simulating the Lyman alpha (Ly alpha) absorption optical depth in presence of neutral hydrogen 'islands' left over from reionization at redshifts 5 less than or similar to z less than or similar to 6. The main inputs to the analysis are (i) a semi-numerical photon-conserving model of ionized regions during reionization (named script) along with a prescription for simulating the shadowing by neutral islands and (ii) the fluctuating Gunn-Peterson approximation to model the Ly alpha absorption. Our model is then used for simulating the large-scale fluctuations in the effective optical depth as observed along sightlines towards high-z quasars. Our model is fully described by five parameters. By setting two of them to default values and varying the other three, we obtain the constraints on reionization history at 5 less than or similar to z less than or similar to 6 as allowed by the data. We confirm that reionization is not complete before z similar to 5.6 at greater than or similar to 2 sigma confidence, with the exact confidence limits depending on how the non-detections of the flux in the data are treated. We also confirm that the completion of reionization can be as late as z similar to 5.2. With further improvements in the model and with more sightlines at z similar to 6, we can take advantage of the computational efficiency of our analysis to obtain more stringent constraints on the ionization fraction at the tail end of reionization.

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