A Universal Energy Distribution for FRB 121102

Abstract

Fast radio bursts (FRBs) are millisecond radio transients with large dispersion measures. An outstanding question is the relation between repeating FRBs and those with a single burst. In this paper, we study the energy distribution of the repeating FRB 121102. For a power-law distribution of energy , we show that the value of α E is in a narrow range 1.6–1.8 for bursts observed by different telescopes at different frequencies, which indicates a universal energy distribution for FRB 121102. Interestingly, a similar power-law index of energy distribution for nonrepeating FRBs observed by Parkes and ASKAP is also found. However, if low-energy bursts below the completeness threshold of Arecibo are discarded for FRB 121102, the slope could be up to 2.2. Implications of such a universal energy distribution are discussed.