The SMBH spin changes the predicted merger time of a nearby stellar-mass binary black hole by 14 to 25 percent and produces a LISA-distinguishable gravitational waveform in a representative Galactic-Center-like example.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Impact of a Spinning Supermassive Black Hole on the Orbit and Gravitational Waves of a Nearby Compact Binary
The SMBH spin changes the predicted merger time of a nearby stellar-mass binary black hole by 14 to 25 percent and produces a LISA-distinguishable gravitational waveform in a representative Galactic-Center-like example.