1. A probe of the maximum energetics of fast radio bursts through a prolific repeating source
- Author
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Ould-Boukattine, O. S., Chawla, P., Hessels, J. W. T., Cooper, A. J., Gawroński, M. P., Herrmann, W., Kirsten, F., Hewitt, D. M., Konijn, D. C., Nimmo, K., Pleunis, Z., Puchalska, W., and Snelders, M. P.
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
Fast radio bursts (FRBs) are sufficiently energetic to be detectable from luminosity distances up to at least seven billion parsecs (redshift $z > 1$). Probing the maximum energies and luminosities of FRBs constrains their emission mechanism and cosmological population. Here we investigate the maximum energetics of a highly active repeater, FRB 20220912A, using 1,500h of observations. We detect $130$ high-energy bursts and find a break in the burst energy distribution, with a flattening of the power-law slope at higher energy. This is consistent with the behaviour of another highly active repeater, FRB 20201124A. Furthermore, we model the rate of the highest-energy bursts and find a turnover at a characteristic spectral energy density of $E^{\textrm{char}}_{\nu} = 2.09^{+3.78}_{-1.04}\times10^{32}$ erg/Hz. This characteristic maximum energy agrees well with observations of apparently one-off FRBs, suggesting a common physical mechanism for their emission. The extreme burst energies push radiation and source models to their limit., Comment: Comments welcome
- Published
- 2024