Compact binary coalescences: Astrophysical processes and lessons learned
On 11 February 2016, the LIGO and Virgo scientific collaborations announced the first direct
detection of gravitational waves, a signal caught by the LIGO interferometers on 14 …
detection of gravitational waves, a signal caught by the LIGO interferometers on 14 …
Population properties of compact objects from the second LIGO–Virgo gravitational-wave transient catalog
R Abbott, TD Abbott, S Abraham… - The Astrophysical …, 2021 - iopscience.iop.org
We analyze the population properties of black holes (BHs) and neutron stars (NSs) in
compact binary systems using data from the LIGO–Virgo Gravitational-Wave Transient …
compact binary systems using data from the LIGO–Virgo Gravitational-Wave Transient …
Properties and astrophysical implications of the 150 M⊙ binary black hole merger GW190521
R Abbott, TD Abbott, S Abraham… - The Astrophysical …, 2020 - iopscience.iop.org
Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational wave astronomy
Galactic nuclei harbouring a central supermassive black hole (SMBH), possibly surrounded
by a dense nuclear cluster (NC), represent extreme environments that house a complex …
by a dense nuclear cluster (NC), represent extreme environments that house a complex …
One channel to rule them all? Constraining the origins of binary black holes using multiple formation pathways
The second LIGO–Virgo catalog of gravitational-wave (GW) transients has more than
quadrupled the observational sample of binary black holes. We analyze this catalog using a …
quadrupled the observational sample of binary black holes. We analyze this catalog using a …
GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal
GW190521: Orbital Eccentricity and Signatures of Dynamical Formation in a Binary Black Hole
Merger Signal - IOPscience This site uses cookies. By continuing to use this site you agree to …
Merger Signal - IOPscience This site uses cookies. By continuing to use this site you agree to …
Properties and Astrophysical Implications of the 150 M o˙ Binary Black Hole Merger GW190521
LIGO Scientific Collaboration… - Astrophysical …, 2020 - researchoutput.csu.edu.au
The gravitational-wave signal GW190521 is consistent with a binary black hole (BBH)
merger source at redshift 0.8 with unusually high component masses, 85-14+ 21 M o and 66 …
merger source at redshift 0.8 with unusually high component masses, 85-14+ 21 M o and 66 …
Post-newtonian dynamics in dense star clusters: Highly eccentric, highly spinning, and repeated binary black hole mergers
We present models of realistic globular clusters with post-Newtonian dynamics for black
holes. By modeling the relativistic accelerations and gravitational-wave emission in isolated …
holes. By modeling the relativistic accelerations and gravitational-wave emission in isolated …
Eccentric black hole mergers forming in globular clusters
J Samsing - Physical Review D, 2018 - APS
We derive the probability for a newly formed binary black hole (BBH) to undergo an
eccentric gravitational wave (GW) merger during binary-single interactions inside a stellar …
eccentric gravitational wave (GW) merger during binary-single interactions inside a stellar …
Eccentric black hole mergers in dense star clusters: The role of binary–binary encounters
We present the first systematic study of strong binary–single and binary–binary black hole
(BH) interactions with the inclusion of general relativity. By including general relativistic …
(BH) interactions with the inclusion of general relativity. By including general relativistic …