A PBH fraction of about 0.1 as dark matter, with 1% in stellar-mass range, produces the observed SGWB amplitude via dynamical friction and hierarchical mergers while explaining JWST early SMBHs.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
representative citing papers
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
Annual variations in scintillation parameters for PSR J0814+7429 reveal an anisotropic scattering screen located 0.23 kpc from Earth at the Local Bubble boundary.
A modified asymmetric broad line region model shows that time-evolving single-BH configurations do not contaminate algorithms searching for massive black hole binaries in multi-epoch spectroscopic data.
citing papers explorer
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Primordial Black Hole contribution to the stochastic background of Gravitational Waves
A PBH fraction of about 0.1 as dark matter, with 1% in stellar-mass range, produces the observed SGWB amplitude via dynamical friction and hierarchical mergers while explaining JWST early SMBHs.
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Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
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Pulsar scintillation studies with LOFAR III. Annual variations in PSR~J0814$+$7429
Annual variations in scintillation parameters for PSR J0814+7429 reveal an anisotropic scattering screen located 0.23 kpc from Earth at the Local Bubble boundary.
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Can a time evolving, asymmetric broad line region mimic a massive black hole binary?
A modified asymmetric broad line region model shows that time-evolving single-BH configurations do not contaminate algorithms searching for massive black hole binaries in multi-epoch spectroscopic data.