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Impact of the reduced speed of light approximation on the post-overlap neutral hydrogen fraction in numerical simulations of the epoch of reionization

机译:在电离时代数值模拟中,光近似速度降低对重叠后中性氢分数的影响

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Context . The reduced speed of light approximation is used in a variety of simulations of the epoch of reionization and galaxy formation. Its popularity stems from its ability to drastically reduce the computing cost of a simulation by allowing the use of larger and therefore fewer timesteps to reach a solution. This approximation is physically motivated by the fact that ionization fronts rarely propagate faster than some fraction of the speed of light. However, no global proof of the physical validity of this approach is available and possible artefacts resulting from this approximation therefore need to be identified and characterized to allow its proper use. Aims . In this paper we investigate the impact of the reduced speed of light approximation on the predicted properties of the intergalactic medium. Methods . To this end we used fully coupled radiation-hydrodynamics RAMSES-CUDATON simulations of the epoch of reionization. Results . We find that reducing the speed of light by a factor 5 (20, 100) leads to overestimating the post-reionization average volume-weighted neutral hydrogen fraction by a similar factor ~5 (20, 100) with respect to full speed of light simulations. We show that the error is driven by the hydrogen – photon chemistry by considering the analytical solution for a strongly ionized hydrogen gas in photoionization equilibrium. In this regime, reducing the speed of light has the same effect as artificially reducing the photon density or the hydrogen photoionization cross section and leads to an underestimated ionizing intensity. We confirm this interpretation by running additional simulations using a reduced speed of light in the photon propagation module, but this time we keep the true speed of light in the chemistry module. With this set-up, the post-reionization neutral hydrogen fractions converge to the full speed of light value, which validates our explanation. Increasing spatial resolution beyond a cell size of 1 kpc physical, so as to better resolve Lyman-limit systems, does not significantly affect our conclusions.
机译:语境。降低的光逼近速度可用于电离和星系形成时代的各种模拟。它之所以流行,是因为它具有通过允许使用更大,因此更少的时间步长来获得解决方案的能力,从而大大降低了模拟的计算成本。这种近似在物理上是受以下事实驱使的:电离前沿很少传播得快于光速的几分之一。但是,尚无有关该方法物理有效性的全球证明,因此需要确定和近似化由此近似所导致的可能伪影,并对其特征进行表征,以使其能够正确使用。目的。在本文中,我们研究了降低的光逼近速度对星系间介质预测特性的影响。方法 。为此,我们使用了电离时代的完全耦合的辐射流体动力学RAMSES-CUDATON模拟。结果。我们发现,将光速降低5倍(20,100)会导致相对于全光模拟,将电离后平均体积加权的中性氢分数高估约5倍(20,100)。 。通过考虑光离子化平衡中强电离氢气的分析解决方案,我们证明了误差是由氢-光子化学驱动的。在这种情况下,降低光速具有与人为降低光子密度或氢光电离截面相同的效果,并导致电离强度被低估。我们通过使用光子传播模块中降低的光速运行其他模拟来确认这种解释,但是这次我们在化学模块中保留了真实的光速。通过这种设置,电离后的中性氢馏分会聚到全光速值,这证实了我们的解释。将空间分辨率提高到超过1 kpc物理像元大小,以更好地解析Lyman极限系统,不会显着影响我们的结论。

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