5D rotating PBHs in the Dark Dimension with memory burden produce a stochastic GW background peaking at nHz to Hz frequencies, detectable by future observatories within the mass window 10^10 to 10^21 g.
Gravitational waves induced by scalar perturbations as probes of the small-scale primordial spectrum.Phys
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Secondary Gravitational Wave Signatures from 5D Rotating Primordial Black Holes in the Dark Dimension
5D rotating PBHs in the Dark Dimension with memory burden produce a stochastic GW background peaking at nHz to Hz frequencies, detectable by future observatories within the mass window 10^10 to 10^21 g.