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.
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Stellar-mass primordial black holes have minor impact on primordial star formation while supermassive ones can seed massive early structures explaining apparent overabundance of high-redshift galaxies.
citing papers explorer
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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.
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Impact of primordial black holes on the formation of the first stars and galaxies
Stellar-mass primordial black holes have minor impact on primordial star formation while supermassive ones can seed massive early structures explaining apparent overabundance of high-redshift galaxies.