Forecasts for Helium Reionization Detection with Fast Radio Bursts in the Era of Square Kilometre Array
Jun-Jie Wei, Chong-Yu Gao

TL;DR
This paper forecasts the ability of the upcoming SKA to detect and constrain the epoch of He II reionization using dispersion measures of a large sample of FRBs, showing high detection significance and precise redshift estimates.
Contribution
It provides the first quantitative forecast of He II reionization detection significance using FRB data from SKA, including detailed signal-to-noise and redshift uncertainty estimates.
Findings
Detection significance can reach 32-50 sigma with SKA FRB data.
Uncertainty in reionization redshift can be constrained to 0.022-0.031.
The impact of different reionization redshift models on forecasts is modest.
Abstract
The observed dispersion measures (DMs) of fast radio bursts (FRBs) are a good indicator of the amount of ionized material along the propagation paths. In this work, we present a forecast of He II reionization detection using the DM and redshift measurements of FRBs from the upcoming Square Kilometre Array (SKA). Assuming a model of the Universe in which He II reionization occurred at a specific redshift , we analyze what extent the signal-to-noise ratio () for the detection of the amplitude of reionization can be achieved in the era of SKA. Using mock FRB data from a one-year observation of the second phase of SKA, we find that the for detecting He II reionization can approach the level and the uncertainty on the reionization redshift can be constrained to be , depending on the assumed…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Atomic and Subatomic Physics Research
