Abstract

The highest brightness temperature ever observed are from "nanoshots" from the Crab pulsar which we argue could be the signature of bursts of vacuum e±e^{\pm} pair production. If so this would be the first time the astronomical Schwinger effect has been observed. These "Schwinger sparks" would be an intermittent but extremely powerful, $\sim 10^3 L_{\astrosun}$, 10 PeV e±e^{\pm} accelerator in the heart of the Crab. These nanosecond duration sparks are generated in a volume less than 1m31 m^3 and the existence of such sparks has implications for the small scale structure of the magnetic field of young pulsars such as the Crab. This mechanism may also play a role in producing other enigmatic bright short radio transients such as fast radio bursts.

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