TL;DR
This paper proposes that macroscopic dark matter could produce uniquely straight lightning channels in thunderstorms, offering a new observational signature to detect or constrain such dark matter candidates.
Contribution
It introduces the idea that macro-induced lightning would be extremely straight and distinct, and estimates the observational parameter space using Earth and Jupiter data.
Findings
Macro-induced lightning would be highly straight and distinguishable from ordinary lightning.
The parameter space for macro detection via lightning is estimated based on thunderstorm frequency.
Potential to probe macro properties through Earth and Jupiter lightning observations.
Abstract
Macroscopic dark matter (macros) is a broad class of alternative candidates to particle dark matter. These candidates would transfer energy to matter primarily through elastic scattering. A sufficiently large macro passing through the atmosphere would produce a straight channel of ionized plasma. If the cross-section of the macro is , then under atmospheric conditions conducive to lightning (eg. a thunderstorm) the plasma channel would be sufficient to seed a lightning strike with a single leader. This is entirely unlike ordinary bolt lightning in which a long sequence of hundreds or thousands of few-meter-long leaders are strung together. This macro-induced lightning would be extremely straight, and thus highly distinctive. Neither wind shear nor magnetohydrodynamic instabilities would markedly spoil its straightness. The only photographically…
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