Eccentric black hole gravitational-wave capture sources in galactic nuclei: Distribution of binary parameters
Mergers of binary black holes on eccentric orbits are among the targets for second-generation ground-based gravitational-wave detectors. These sources may commonly form in galactic nuclei due to gravitational-wave emission during close flyby events of single objects. We determine the distributions o...
Main Authors: | Gondan, L, Kocsis, B, Raffai, P, Frei, Z |
---|---|
Format: | Journal article |
Language: | English |
Published: |
IOP Publishing
2018
|
Similar Items
-
Accuracy of estimating highly eccentric binary black hole parameters with gravitational-wave detections
by: Gondán, L, et al.
Published: (2018) -
High eccentricities and high masses characterize gravitational-wave captures in galactic nuclei as seen by Earth-based detectors
by: Gondan, L, et al.
Published: (2021) -
Measurement accuracy of inspiraling eccentric neutron star and black hole binaries using gravitational waves
by: Gondan, L, et al.
Published: (2019) -
Astrophysical gravitational-wave echoes from galactic nuclei
by: Gondán, L, et al.
Published: (2022) -
Eccentric black hole mergers in active galactic nuclei
by: Tagawa, H, et al.
Published: (2021)