Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

While most of the compact-binary mergers detected by LIGO and Virgo are expected to
consist of first-generation black holes formed from the collapse of stars, others might instead …

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 …

The detection of gravitational waves by Advanced LIGO and Advanced Virgo provides an
opportunity to test general relativity in a regime that is inaccessible to traditional …

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 …

The recently established formalism of a worldline quantum field theory, which describes the
classical scattering of massive bodies (black holes, neutron stars, or stars) in Einstein …

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 …

We explore hierarchical black hole (BH) mergers in nuclear star clusters (NSCs), globular
clusters (GCs) and young star clusters (YSCs), accounting for both original and dynamically …

The origin of black hole mergers discovered by the LIGO and Virgo gravitational-wave
observatories is currently unknown. GW190521, is the heaviest black hole merger detected …