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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
Dissertation investigates gravitational waves produced during cosmic inflation as a possible origin for the nanohertz stochastic background sought by NANOGrav.
citing papers explorer
-
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.
-
Gravitational Waves from the Big Bang
Dissertation investigates gravitational waves produced during cosmic inflation as a possible origin for the nanohertz stochastic background sought by NANOGrav.