Statistical properties and cosmological applications of fast radio bursts

TL;DR

This paper reviews the statistical properties of fast radio bursts (FRBs) and their applications in cosmology, highlighting recent observational advances and how FRBs can probe cosmic baryons, reionization, and gravitational lensing.

Contribution

It provides a comprehensive summary of recent statistical analyses and cosmological uses of large FRB samples, emphasizing new insights gained from accumulated observational data.

Findings

FRB energy functions and waiting time distributions analyzed

FRBs used to probe missing baryons and circumgalactic medium

FRBs contribute to measurements of cosmological parameters and reionization history

Abstract

Fast radio burst (FRB) is a type of extragalactic radio signal characterized by millisecond duration, extremely high brightness temperature, and large dispersion measure. It remains a mystery in the universe. Advancements in instrumentation have led to the discovery of 816 FRB sources and 7622 bursts from 67 repeating FRBs now. This field is undergoing rapid development, rapidly advancing our understanding of the physics of FRBs as new observational data accumulates. The accumulation of data has also promoted our exploration of our universe. In this review, we summarize the statistical analysis and cosmological applications using large samples of FRBs, including the energy functions, the waiting time distributions of repeating FRBs, the probe of "missing baryons" and circumgalactic medium in the universe, measurements of cosmological parameters, exploration of the epoch of reionization history, and study of the gravitational lensing of FRBs.