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Ultralight Primordial Black Holes
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The fate of ultralight black holes depends on whether or not evaporation stops at or around the Planck scale. If evaporation stops, the general expectation is that a population of Planck-scale will be left over, possibly including a significant fraction of electrically charged relics. If evaporation does not stop, a runaway "explosion" would occur, with significant and potentially detectable high-energy emission. Here, I review both possibilities, with an emphasis on current status and future detection prospects.
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Cited by 2 Pith papers
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Comprehensively Constraining Ultra-Light Primordial Black Holes Through Relic Formation and Early Mergers
Ultra-light primordial black holes that evaporate before Big Bang nucleosynthesis can still be probed through Planck-mass relics and early binary mergers, leaving a narrow window where relics make up all dark matter.
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Picolensing as a Probe of Primordial Black Hole Dark Matter
Asteroid-mass primordial black hole dark matter could be probed by picolensing of gamma-ray bursts, but only with detector separations of at least Earth-L2 distance once realistic GRB size uncertainties are included.
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