Constraining the epoch of reionization with highly dispersed fast radio bursts
نویسندگان
چکیده
The period in which hydrogen the intergalactic medium (IGM) is ionized, known as Epoch of Reionization (EoR) still poorly understood. timing and duration EoR expected to be governed by underlying astrophysics. Furthermore, most models reionization predict a correlation between density ionization field. Here we consider using mean dispersion measure (DM) high redshift Fast Radio Bursts (FRBs) probe astrophysics morphology EoR. To do this, forecast observational scenarios building mock data sets non-repeating FRBs redshifts $8\leq z \leq 10$. It assumed that all have accompanying spectroscopic measurements. We find samples 100 FRBs, above mentioned narrow range, can rule out uncorrelated at $68\%$ credibility, while larger samples, $\geq 10^4$ $95\%$ credibility. also where Universe entirely neutral $z = 10$ with Further 10^5$ constrain $\Delta z$ (duration ionized fraction 0.25 0.75) 2.0^{+0.5}_{-0.4}$, midpoint 7.8^{+0.4}_{-0.2}$
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2021
ISSN: ['0035-8711', '1365-8711', '1365-2966']
DOI: https://doi.org/10.1093/mnras/stab1438