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Electromagnetic Signatures From Primordial Black Holes in the Solar System
cosmology-and-nongalactic-astrophysicshigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenology
Primordial black holes (PBHs) in the asteroid-mass range, with typical masses $10^{17}\,{\rm g}\lesssim M \lesssim 10^{23}\,{\rm g}$, have drawn significant recent attention as a viable dark matter candidate. The peak frequencies of photons emitted via Hawking radiation from asteroid-mass PBHs range
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