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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
verdicts
UNVERDICTED 3representative citing papers
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
-
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.
-
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.
-
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.