paper

Extracting host galaxy dispersion measure and constraining cosmological parameters using fast radio burst data

arXiv:1608.08154 · doi:10.3847/2041-8205/830/2/L31

Abstract

The excessive dispersion measures (DMs) and high Galactic latitudes of fast radio bursts (FRBs) hint toward a cosmological origin of these mysterious transients. Methods of using measured DM and redshift to study cosmology have been proposed, but one needs to assume a certain amount of DM contribution from the host galaxy (DM) in order to apply those methods. We introduce a slope parameter (where DM is the observed DM subtracting the Galactic contribution), which can be directly measured when a sample of FRBs have measured. We show that can be roughly inferred from and the mean values, and , of the sample. Through Monte Carlo simulations, we show that the mean value of local host galaxy DM, , along with other cosmological parameters (mass density in the CDM model, and the IGM portion of the baryon energy density ) can be independently measured through MCMC fitting to the data.

7 pages, 5 figures, Accepted for publication in ApJL

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