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- W2023962879 abstract "Formation of primordial black holes (PBHs) requires a large root-mean-square amplitude of density fluctuations, which generate second-order tensor perturbations that can be compared with observational constraints. We show that pulsar timing data essentially rules out PBHs with 10 2–4 M ⊙ which were previously considered as a candidate of intermediate-mass black hoes and that PBHs with mass range 10 20–25 g which provide an astrophysical candidate for dark matter may be probed by future space-based laser interferometers." @default.
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- W2023962879 date "2011-01-01" @default.
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- W2023962879 title "GRAVITATIONAL-WAVE CONSTRAINTS ON ABUNDANCE OF PRIMORDIAL BLACK HOLES" @default.
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- W2023962879 doi "https://doi.org/10.1142/s2010194511000171" @default.
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