Intergalactic medium dispersion measures of fast radio bursts estimated from IllustrisTNG simulation and their cosmological applications
arXiv:2011.14494 · doi:10.3847/1538-4357/abceb9
Abstract
Fast radio bursts (FRBs) are millisecond-duration radio transients and can be used as a cosmological probe. However, the dispersion measure (DM) contributed by intergalactic medium (IGM) is hard to be distinguished from other components. In this paper, we use the IllustrisTNG simulation to realistically estimate the up to . We find pc cm at . The probability distribution of can be well fitted by a quasi-Gaussian function with a long tail. The tail is caused by the structures along the line of sight in IGM. Subtracting DM contributions from the Milky Way and host galaxy for localized FRBs, the value is close to the derived relation. We also show the capability to constrain the cosmic reionization history with the of high-redshift FRBs in the IllustrisTNG universe. The derived relation at high redshifts can be well fitted by a reionization model with the reionization redshift , which is compatible with the reionization model used by the IllustrisTNG simulation. The of high-redshift FRBs also provides an independent way to measure the optical depth of cosmic microwave background (CMB). Our result can be used to derive the pseudo-redshifts of non-localized FRBs for \ \ pc cm.
10 pges, 1 table, accepted for publication in ApJ
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Cited by in corpus (4)
- Finding the missing baryons in the intergalactic medium with localized fast radio bursts
- Deep Synoptic Array science: Two fast radio burst sources in massive galaxy clusters
- A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
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