Fast Radio Burst Breakouts from Magnetar Burst Fireballs
arXiv:2008.01114 · doi:10.3847/2041-8213/abc6a3
Abstract
The recent discovery of a Mega-Jansky radio burst occurring simultaneously with short X-ray bursts from the Galactic magnetar (strongly magnetized neutron star (NS)) SGR 1935+2154 is a smoking gun for the hypothesis that some cosmological fast radio bursts (FRBs) arise from magnetar bursts. We argue that the X-ray bursts with high temperature keV entail an electron--positron () outflow from a trapped--expanding fireball, polluting the NS magnetosphere before the FRB emission. The outflow is opaque to FRB photons, and is strongly Compton-dragged by the X-ray bursts. Nevertheless, the FRB photons can break out of the outflow with radiation forces if the FRB emission radius is larger than a few tens of NS radii. A FRB is choked if the FRB is weaker or the X-ray bursts are stronger, possibly explaining why there are no FRBs with giant flares and no detectable X-ray bursts with weak FRBs. We also speculate that the outflow may be inevitable for FRBs, solving the problem of why the FRBs occur only with high- X-ray bursts. The breakout physics is important for constraining the emission mechanism and electromagnetic counterparts to future FRBs.
9 pages, 3 figures, accepted for publication in ApJ Letter
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Cited by in corpus (22)
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