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20242026
most citedNonlinear quasinormal mode detectability with next-generation gravitational wave detectors

40 citations · 118 across the 20 of their papers we have counts for

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5 papers · 1 filter

astro-ph.CO2025★ 7 cited

Primordial Black-Hole-Based Pathways to Little Red Dots

Valerio De Luca, Loris Del Grosso, Gabriele Franciolini +4

The James Webb Space Telescope has uncovered a population of compact, high-redshift sources, the Little Red Dots (LRDs), which may host supermassive black holes (BHs) significantly…

astro-ph.GA2025★ 1 cited

Milky Way Globular Clusters: Nurseries for Dynamically-Formed Binary Black Holes

Federico Angeloni, Konstantinos Kritos, Raffaella Schneider +4

We present a novel self-consistent theoretical framework to characterize the formation, evolution, and merger sites of dynamically-formed black hole binaries, with a focus on expla…

gr-qc2025

Coincident morphological transitions in precessing black-hole binaries

Davide Gerosa, Giulia Foroni, Giulia Fumagalli +1

We present new insights into the phenomenology of post-Newtonian spin precession in black-hole binaries. Using multi-timescale methods, previous work has shown that the precession…

gr-qc2025★ 8 cited

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★ 2 cited

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…