Do Multi-Structural One-Off FRBs Trace Similar Cosmology History with Repeaters?

Author:

Zhu Yuhao12ORCID,Niu Chenhui3ORCID,Cui Xianghan12ORCID,Li Di124ORCID,Feng Yi5ORCID,Tsai Chaowei1ORCID,Wang Pei1ORCID,Zhang Yongkun12ORCID,Meng Fanyi2ORCID,Zheng Zheng1

Affiliation:

1. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China

2. University of Chinese Academy of Sciences, Beijing 100049, China

3. Institute of Astrophysics, Central China Normal University, Wuhan 430079, China

4. NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa

5. Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou 311100, China

Abstract

Fast Radio Bursts (FRBs) are millisecond-duration transient events that are typically observed at radio wavelengths and cosmological distances but their origin remains unclear. Furthermore, most FRB origin models are related to the processes at stellar scales, involving neutron stars, blackholes, supernovae, etc. In this paper, our purpose is to determine whether multi-structural one-off FRBs and repeaters share similarities. To achieve this, we focus on analyzing the relationship between the FRB event rate and the star formation rate, complemented by statistical testing methods. Based on the CHIME/FRB Catalog 1, we calculate the energy functions for four subsamples, including apparent non-repeating FRBs (one-offs), repeaters, multi-structural one-offs, and the joint repeaters and multi-structural events, respectively. We then derive the FRB event rates at different redshifts for all four subsamples, all of which were found to share a similar cosmological evolution trend. However, we find that the multi-structural one-offs and repeaters are distinguishable from the KS and MWW tests.

Funder

National Natural Science Foundation of China

National SKA Program of China

Office the leading Group for Cyberspace Affairs, CAS

NSFC

China Manned Space Project

Publisher

MDPI AG

Subject

General Physics and Astronomy

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