The motion of the centre of mass of a coalescing binary black hole (BBH) in a gravitational
potential, imprints a line-of-sight acceleration (LOSA) on to the emitted gravitational-wave …

The LIGO-Virgo analysis of the signals from compact binary mergers observed so far have
assumed in-vacuum isolated binary systems, neglecting the potential presence of …

We describe an implementation of the relative binning technique to speed up parameter
estimation of gravitational-wave signals. We first give a pedagogical overview of relative …

General relativity (GR) has proven to be a highly successful theory of gravity since its
inception. The theory has thrivingly passed numerous experimental tests, predominantly in …

The LIGO-Virgo analyses of signals from compact binary mergers observed so far have
assumed isolated binary systems in a vacuum, neglecting the potential presence of …

The dense and dynamic environments within active galactic nuclei (AGN) accretion disks
may serve as prolific birthplaces for binary black holes (BBHs) and one possible origin for …

Galactic double white dwarf (DWD) binaries are among the guaranteed sources for the
Laser Interferometer Space Antenna (LISA), an upcoming space-based gravitational wave …

The dense and dynamic environments within active galactic nuclei (AGN) accretion disks
may serve as prolific birthplaces for binary black holes (BBHs) and one possible origin for …

Asymmetric emission of gravitational waves during a compact binary coalescence results in
the loss of linear momentum and a corresponding “kick” or recoil on the binary's center of …

Recent astrophysical models predict that stellar-mass binary black holes (BBHs) could form
and coalesce within a few gravitational radii of a supermassive black hole (SMBH) …