Exact non-singular black holes from the phantom DBI field evaporate to gram-mass relics, opening a new mass window for primordial black holes as dark matter.
In the unitsa=B= G= 1 (whereκ 2 = 8π), the scalar field approachesϕ(r→ ∞) = 1 8πϵ(π−6M)
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Exact, non-singular black holes from a phantom DBI Field as primordial dark matter
Exact non-singular black holes from the phantom DBI field evaporate to gram-mass relics, opening a new mass window for primordial black holes as dark matter.