Impact of the Epoch of Reionization sources on the 21-cm bispectrum
Leon Noble, Mohd Kamran, Suman Majumdar, Chandra Shekhar Murmu,, Raghunath Ghara, Garrelt Mellema, Ilian T. Iliev, Jonathan R. Pritchard

TL;DR
This paper investigates how different sources of ionizing radiation during the Epoch of Reionization influence the 21-cm bispectrum, demonstrating its potential to distinguish between various reionization scenarios and IGM morphologies.
Contribution
It presents the first comprehensive analysis of the 21-cm bispectrum across multiple reionization models, showing its effectiveness in differentiating IGM morphologies.
Findings
Significant differences in bispectrum magnitude and sign across reionization scenarios.
Large-scale bispectrum can distinguish inside-out, outside-in, and mixed morphologies.
Specific $k$-triangle shapes enhance the ability to differentiate scenarios.
Abstract
The morphology of the 21-cm signal emitted by the neutral hydrogen present in the intergalactic medium (IGM) during the Epoch of Reionization (EoR) depends both on the properties of the sources of ionizing radiation and on the underlying physical processes within the IGM. Variation in the morphology of the IGM 21-cm signal due to the different sources of the EoR is expected to have a significant impact on the 21-cm bispectrum, which is one of the crucial observable statistics that can evaluate the non-Gaussianity present in the signal and which can be estimated from radio interferometric observations of the EoR. Here we present the 21-cm bispectrum for different reionization scenarios assuming different simulated models for the sources of reionization. We also demonstrate how well the 21-cm bispectrum can distinguish between different IGM 21-cm signal morphologies, arising due to the…
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Taxonomy
TopicsTerahertz technology and applications
