paper

A universal energy distribution for FRB 121102

arXiv:1904.12408 · doi:10.3847/1538-4357/ab35dc

Abstract

Fast radio bursts (FRBs) are milliseconds radio transients with large dispersion measures (DMs). 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 is in a narrow range for bursts observed by different telescopes at different frequencies, which indicates a universal energy distribution for FRB 121102. Interestingly, similar power-law index of energy distribution for non-repeating FRBs observed by Parkes and ASKAP is also found. However, if low-energy bursts below 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.

arXiv comment17 pages, 3 figures, 8 tables, accepted for publication in ApJ

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