activity
20242026
collaborators

5 papers

gr-qc2026

Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors

Francesco Iacovelli, Luca Reali, Emanuele Berti +3

Next-generation (XG) gravitational-wave detectors, such as Cosmic Explorer (CE) and the Einstein Telescope (ET), will observe compact binary coalescences at unprecedented rates and…

gr-qc2025

Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors

Haowen Zhong, Luca Reali, Bei Zhou +2

Cosmological gravitational-wave backgrounds are an exciting science target for next-generation ground-based detectors, as they encode invaluable information about the primordial Un…

astro-ph.HE2025

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers

Konstantinos Kritos, Luca Reali, Ken K. Y. Ng +2

Next-generation ground-based gravitational wave observatories will observe mergers of intermediate-mass black holes (IMBHs) out to high redshift. Such IMBHs can form through runawa…

gr-qc2025

Possible Causes of False General Relativity Violations in Gravitational Wave Observations

Anuradha Gupta, K. G. Arun, Enrico Barausse +40

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 w…

astro-ph.HE2024

Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters

Konstantinos Kritos, Luca Reali, Davide Gerosa +1

The spin of intermediate-mass black holes (IMBHs) growing through repeated black hole mergers in stellar clusters statistically asymptotes to zero. Putative observations of IMBHs w…