The shape and size distribution of H ii regions near the percolation transition

Bag, Satadru ; Mondal, Rajesh ; Sarkar, Prakash ; Bharadwaj, Somnath ; Sahni, Varun (2018) The shape and size distribution of H ii regions near the percolation transition Monthly Notices of the Royal Astronomical Society, 477 (2). pp. 1984-1992. ISSN 0035-8711

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Official URL: http://doi.org/10.1093/mnras/sty714

Related URL: http://dx.doi.org/10.1093/mnras/sty714

Abstract

Using Shapefinders, which are ratios of Minkowski functionals, we study the morphology of neutral hydrogen (H I) density fields, simulated using seminumerical technique (inside-out), at various stages of reionization. Accompanying the Shapefinders, we also employ the ‘largest cluster statistic’ (LCS), originally proposed in Klypin & Shandarin, to study the percolation in both neutral and ionized hydrogen. We find that the largest ionized region is percolating below the neutral fraction xHI≲0.728 (or equivalently z ≲ 9). The study of Shapefinders reveals that the largest ionized region starts to become highly filamentary with non-trivial topology near the percolation transition. During the percolation transition, the first two Shapefinders – ‘thickness’ (T) and ‘breadth’ (B) – of the largest ionized region do not vary much, while the third Shapefinder – ‘length’ (L) – abruptly increases. Consequently, the largest ionized region tends to be highly filamentary and topologically quite complex. The product of the first two Shapefinders, T × B, provides a measure of the ‘cross-section’ of a filament-like ionized region. We find that, near percolation, the value of T × B for the largest ionized region remains stable at ∼7 Mpc2 (in comoving scale) while its length increases with time. Interestingly, all large ionized regions have similar cross-sections. However, their length shows a power-law dependence on their volume, L ∝ V0.72, at the onset of percolation.

Item Type:Article
Source:Copyright of this article belongs to The Royal Astronomical Society.
Keywords:Intergalactic Medium; Dark Ages; Reionization; First Stars; Large-Scale Structure Of Universe; Cosmology: Theory.
ID Code:116294
Deposited On:09 Apr 2021 04:28
Last Modified:09 Apr 2021 04:28

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