Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations
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| Formato: | Preprint |
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2023
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| _version_ | 1866915440449552384 |
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| author | Pramanick, Suman Mondal, Rajesh Bharadwaj, Somnath |
| author_facet | Pramanick, Suman Mondal, Rajesh Bharadwaj, Somnath |
| contents | The Epoch of Reionization (EoR) neutral Hydrogen (HI) 21-cm signal evolves significantly along the line-of-sight (LoS) due to the light-cone (LC) effect. It is important to accurately incorporate this in simulations in order to correctly interpret the signal. The 21-cm LC simulations are typically produced by stitching together slices from a finite number $(N_{\rm RS})$ of "reionization snapshot'', each corresponding to a different stage of reionization. In this paper, we have quantified the errors in the 21-cm LC simulation due to the finite value of $N_{\rm RS}$. We show that this can introduce large discontinuities $(> 200 \%)$ at the stitching boundaries when $N_{\rm RS}$ is small $(=2,4)$ and the mean neutral fraction jumps by $δ\bar{x}_{\rm HI} =0.2,0.1$ respectively at the stitching boundaries. This drops to $17 \%$ for $N_{\rm RS}=13$ where $δ\bar{x}_{\rm HI}=0.02$. We find that we can achieve $δ\bar{x}_{\rm HI} \le 0.01$ with $N_{\rm RS} =26$, and we use this as the reference for comparing the other simulations. We present and also validate a method for mitigating this error by increasing $N_{\rm RS}$ without a proportional increase in the computational costs which are mainly incurred in generating the dark matter and halo density fields. Our method generates these fields only at a few redshifts, and interpolates them to generate reionization snapshots at closely spaced redshifts. We use this to generate 21-cm LC simulations with $N_{\rm RS}=51,101$ and $201$, and show that the errors go down as $N_{\rm RS}^{-1}$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2304_14171 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations Pramanick, Suman Mondal, Rajesh Bharadwaj, Somnath Cosmology and Nongalactic Astrophysics The Epoch of Reionization (EoR) neutral Hydrogen (HI) 21-cm signal evolves significantly along the line-of-sight (LoS) due to the light-cone (LC) effect. It is important to accurately incorporate this in simulations in order to correctly interpret the signal. The 21-cm LC simulations are typically produced by stitching together slices from a finite number $(N_{\rm RS})$ of "reionization snapshot'', each corresponding to a different stage of reionization. In this paper, we have quantified the errors in the 21-cm LC simulation due to the finite value of $N_{\rm RS}$. We show that this can introduce large discontinuities $(> 200 \%)$ at the stitching boundaries when $N_{\rm RS}$ is small $(=2,4)$ and the mean neutral fraction jumps by $δ\bar{x}_{\rm HI} =0.2,0.1$ respectively at the stitching boundaries. This drops to $17 \%$ for $N_{\rm RS}=13$ where $δ\bar{x}_{\rm HI}=0.02$. We find that we can achieve $δ\bar{x}_{\rm HI} \le 0.01$ with $N_{\rm RS} =26$, and we use this as the reference for comparing the other simulations. We present and also validate a method for mitigating this error by increasing $N_{\rm RS}$ without a proportional increase in the computational costs which are mainly incurred in generating the dark matter and halo density fields. Our method generates these fields only at a few redshifts, and interpolates them to generate reionization snapshots at closely spaced redshifts. We use this to generate 21-cm LC simulations with $N_{\rm RS}=51,101$ and $201$, and show that the errors go down as $N_{\rm RS}^{-1}$. |
| title | Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2304.14171 |