collaborators

8 papers

astro-ph.IM2026

LIGO A: Detector Design and Science Prospects Beyond A+

L. Sun, K. Kuns, B. J. J. Slagmolen +1153

We present the LIGO A detector concept, an upgrade for the LIGO observatories based on room-temperature interferometers beyond the fifth observing run (O5). Building on th…

physics.soc-ph2026

The Early Career Workshop of GR-Amaldi 2025

S Al-Shammari, C P L Berry, C E A Chapman-Bird +18

Gravitational physics and astronomy have developed rapidly over the last decade, driven by new observations and theoretical breakthroughs. As new as the science and technology of t…

gr-qc2025

Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches

Sayantan Ghosh, Leigh Smith, Jiyoon Sun +3

All-sky searches for generic short-duration astrophysical GW transients are often challenging because of noise transients. Developing novel signal-noise discriminators is crucial f…

gr-qc2025

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

astro-ph.CO2025

Using gravitational wave dark sirens to choose between host galaxy weighting models

Zhuotao Li, Rachel Gray, Ik Siong Heng

Binary black hole (BBH) mergers,, an important source of gravitational-waves(GWs), are assumed to be hosted in galaxies. The probability of a galaxy to host a BBH is related to its…

gr-qc2025

Search for dynamical black hole captures with Gaussian mixture modelling

Leigh Smith, Shubhanshu Tiwari, Michael Ebersold +3

Gravitational waves (GWs) are expected to originate from black holes interacting dynamically in dense astrophysical environments. In such environments, given that the velocity and…