Within a covariant effective loop quantum gravity model, black holes evaporate asymptotically to a minimum-area remnant of mass ~20.94 μg that cannot form in finite time.
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Loopy Black-Hole Remnants
Within a covariant effective loop quantum gravity model, black holes evaporate asymptotically to a minimum-area remnant of mass ~20.94 μg that cannot form in finite time.