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A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
Khun Sang Phukon, Patricia Schmidt, Geraint Pratten
Compact binaries on eccentric orbits are another class of gravitational-wave (GW) sources that can provide a wealth of information on binary formation pathways and astrophysical en…
Premerger observation and characterization of massive black hole binaries
Gareth Cabourn Davies, Ian Harry, Michael J. Williams +11
We demonstrate an end-to-end technique for observing and characterizing massive black hole binary signals before they merge with the LISA space-based gravitational-wave observatory…
Strong Field Scattering of Black Holes: Assessing Resummation Strategies
Shaun Swain, Geraint Pratten, Patricia Schmidt
Recent developments in post-Minkowksian (PM) calculations have led to a fast-growing body of weak-field perturbative information. As such, there is major interest within the gravit…
What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
Justin Janquart, David Keitel, Rico K. L. Lo +26
On the 29th of May 2023, the LIGO-Virgo-KAGRA Collaboration observed a compact binary coalescence event consistent with a neutron star-black hole merger, though the heavier object…
Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
Alice Spadaro, Riccardo Buscicchio, David Izquierdo-Villalba +3
Massive black-hole binaries will be the loudest sources detectable by LISA. These systems are predicted to form during the hierarchical assembly of cosmic structures and coalesce b…
Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
Natalie Williams, Patricia Schmidt, Geraint Pratten
Gravitational waves from inspiralling binary neutron stars provide unique access to ultra-dense nuclear matter and offer the ability to constrain the currently unknown neutron star…