arXiv (All)
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On the effective spin-mass ratio relation of binary black hole mergers that evolved in isolation
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenasolar-and-stellar-astrophysics
The ground-based measurement of gravitational waves (GW) from merging binary black holes (BBH) allows independent determination of spins of stellar-remnant black holes (BH). The observed population of BBH mergers exhibits two intriguing peculiarities related to BH spins, namely, a positively biased
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