Detecting Helium Reionization with Fast Radio Bursts
arXiv:2001.11517 · doi:10.1103/PhysRevD.101.103019
Abstract
Fast radio bursts (FRB) probe the electron density of the universe along the path of propagation, making high redshift FRB sensitive to the helium reionization epoch. We analyze the signal to noise with which a detection of the amplitude of reionization can be made, and its redshift, for various cases of future FRB survey samples, assessing survey characteristics including total number, redshift distribution, peak redshift, redshift depth, and number above the reionization redshift, as well as dependence on reionization redshift. We take into account scatter in the dispersion measure due to an inhomogeneous intergalactic medium (IGM) and uncertainty in the FRB host and environment dispersion measure, as well as cosmology. For a future survey with 500 FRB extending out to , and a sudden reionization, the detection of helium reionization can approach the level and the reionization redshift be determined to in an optimistic scenario, or and taking into account further uncertainties on IGM fraction evolution and redshift uncertainties.
8 pages, 8 figures; v2 minor clarifications in text and Fig. 3, matches PRD version
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- The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
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- Constraining HeII Reionization Detection Uncertainties via Fast Radio Bursts
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- Reconstruction of Reionization History through Dispersion Measure of Fast Radio Bursts
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- Detecting the signature of helium reionization through 3HeII 3.46cm line-intensity mapping