On the radiation mechanism of repeating fast radio bursts
Wenbin Lu, Pawan Kumar

TL;DR
This paper investigates the radiation mechanisms behind repeating fast radio bursts, concluding that antenna curvature emission powered by magnetar magnetic reconnection is the most plausible explanation for their high luminosity.
Contribution
The study constrains plasma conditions for FRB emission mechanisms and identifies antenna curvature emission as the most viable process, linking it to magnetar activity.
Findings
Maser mechanisms cannot explain high FRB luminosity without unrealistic conditions.
Antenna curvature emission by charge bunches is the most plausible mechanism.
Magnetar magnetospheres may be clumpy, facilitating charge bunch formation.
Abstract
Recent observations show that fast radio bursts (FRBs) are energetic but probably non-catastrophic events occurring at cosmological distances. The properties of their progenitors are largely unknown in spite of many attempts to determine them using the event rate, duration and energetics. Understanding the radiation mechanism for FRBs should provide the missing insights regarding their progenitors, which is investigated in this paper. The high brightness temperatures (>10^{35} K) of FRBs mean that the emission process must be coherent. Two general classes of coherent radiation mechanisms are considered --- maser and the antenna mechanism. We use the observed properties of the repeater FRB 121102 to constrain the plasma conditions needed for these two mechanisms. We have looked into a wide variety of maser mechanisms operating in either vacuum or plasma and find that none of them can…
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