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作 者:Min Meng Qiu-Ju Huang Can-Min Deng
出 处:《Research in Astronomy and Astrophysics》2024年第9期76-82,共7页天文和天体物理学研究(英文版)
基 金:supported by the National Natural Science Foundation of China(NSFC,Grant No.12203013);the Guangxi Science Foundation(grant Nos.2023GXNSFBA026030and Guike AD22035171)。
摘 要:In this paper,we upgrade the constraints for the Earth-mass primordial black hole mergers model based on the first Canadian Hydrogen Intensity Mapping Experiment(CHIME)/fast radio burst(FRB)catalog.Assuming the null hypothesis that the observed non-repeating FRBs originate from Earth-mass primordial black hole mergers,we find that how the charges were distributed in the primordial black hole population is well described by a double powerlaw function with typical charge value of law function with typical charge value of q_(c)/10^(-5)=1.60_(-0.28)^(+0.28),where the power-law index α_(1)=2.33_(-0.18)^(+0.15) for q<q_(c) and α_(2)=4.56_(-0.26)^(+0.30)for q≥q_(c).Here,q represents the charge of the black hole in units of√GM,where M is the mass of the black hole.Furthermore,we infer the local event rate of the bursts is 8.8_(-2.1)^(+5.7)×10^(4)Gpc^(-3) yr^(-1),which indicates that an abundance of the primordial black hole population f■10^(-4) is needed to account for the observed FRBs by CHIME.The results of this paper lay the basis for further research on the electromagnetic radiation background generated by the merger of primordial black hole mergers.
关 键 词:black hole physics (stars:)gamma ray burst:general (cosmology:)dark matter
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