Estimation of H ii Bubble Size Distribution from 21 cm Power Spectrum with Artificial Neural Networks

Author:

Shimabukuro HayatoORCID,Mao YiORCID,Tan JianrongORCID

Abstract

Abstract The bubble size distribution of ionized hydrogen regions probes information about the morphology of H II bubbles during reionization. Conventionally, the H II bubble size distribution can be derived from the tomographic imaging data of the redshifted 21 cm signal from the epoch of reionization, which, however, is observationally challenging even for upcoming large radio interferometer arrays. Given that these interferometers promise to measure the 21 cm power spectrum accurately, we propose a new method, which is based on artificial neural networks, to reconstruct the H II bubble size distribution from the 21 cm power spectrum. We demonstrate that reconstruction from the 21 cm power spectrum can be almost as accurate as being directly measured from the imaging data with fractional error ≲10%, even with thermal noise at the sensitivity level of the Square Kilometre Array. Nevertheless, the reconstruction implicitly exploits the modeling in reionization simulations, and hence the recovered H II bubble size distribution is not an independent summary statistic from the power spectrum, and should be used only as an indicator for understanding H II bubble morphology and its evolution.

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. How informative are summaries of the cosmic 21 cm signal?;Astronomy & Astrophysics;2024-08

2. Probing the intergalactic medium during the Epoch of Reionization using 21 cm signal power spectra;Astronomy & Astrophysics;2024-07

3. Classification and Evaluation System of Oil and Gas Reservoir Based on Artificial Neural Network;2022 International Conference on Artificial Intelligence of Things and Crowdsensing (AIoTCs);2022-10

4. Exploring the cosmic dawn and epoch of reionization with the 21 cm line;Publications of the Astronomical Society of Japan;2022-06-25

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