Fast Afterglows of Fast Radio Bursts
Andrei Gruzinov (NYU)

TL;DR
This paper proposes that fast radio bursts leave behind relativistic plasma that emits observable coherent electromagnetic afterglows, with a predicted decreasing frequency over time, supported by numerical experiments.
Contribution
It introduces a novel model for FRB afterglows based on collisionless plasma relaxation and demonstrates this with numerical simulations.
Findings
Numerical demonstration of fast coherent afterglows.
Predicted afterglow frequency decreases as t^{-3/2}.
Potential observability of FRB afterglows.
Abstract
The main FRB event may leave behind a clump of relativistic plasma with high ``free energy'' density. As the plasma undergoes collisionless relaxation, it emits coherent electromagnetic waves. These electromagnetic waves may be observable as a fast radio afterglow, with decreasing frequency and intensity. We demonstrate the fast coherent afterglow in a numerical experiment. We tentatively predict the peak afterglow frequency decreasing with time as .
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Radio Astronomy Observations and Technology
