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20232026
most citedNonlinear quasinormal mode detectability with next-generation gravitational wave detectors

40 citations · 55 across the 9 of their papers we have counts for

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gr-qc2026

Novel Ringdown Tests of General Relativity with Black Hole Graybody Factors

Romeo Felice Rosato, Francesco Crescimbeni, Sophia Yi +2

We present GreyRing, a new model for the post-merger signal in black-hole binary coalescences based on the graybody factor of the remnant. The model accurately reproduces the full…

gr-qc2026★ 1 cited

Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries

Sophia Yi, Francesco Iacovelli, Emanuele Berti +4

The Laser Interferometer Space Antenna (LISA) will observe massive black hole binaries (MBHBs) with astoundingly high signal-to-noise ratio, leaving parameter estimation with these…

gr-qc2025★ 1 cited

Modeling the frequency-domain ringdown amplitude of comparable-mass mergers with greybody factors

Romeo Felice Rosato, Sophia Yi, Emanuele Berti +1

It was recently shown that, in a binary coalescence, the greybody factor of the remnant black hole modulates the post-merger ringdown signal. In this work, we demonstrate that a si…

gr-qc2025★ 3 cited

Black hole spectroscopy: from theory to experiment

Emanuele Berti, Vitor Cardoso, Gregorio Carullo +65

The "ringdown" radiation emitted by oscillating black holes has great scientific potential. By carefully predicting the frequencies and amplitudes of black hole quasinormal modes a…

gr-qc2025★ 4 cited

Systematic biases in parameter estimation on LISA binaries: The effect of excluding higher harmonics for non-spinning binaries

Sophia Yi, Francesco Iacovelli, Sylvain Marsat +2

The remarkable sensitivity achieved by the planned Laser Interferometer Space Antenna (LISA) will allow us to observe gravitational-wave signals from the mergers of massive black h…

gr-qc2024★ 40 cited

Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors

Sophia Yi, Adrien Kuntz, Enrico Barausse +4

In the aftermath of a binary black hole merger event, the gravitational wave signal emitted by the remnant black hole is modeled as a superposition of damped sinusoids known as qua…

gr-qc2023★ 1 cited

Black hole spectroscopy beyond Kerr: agnostic and theory-based tests with next-generation interferometers

Andrea Maselli, Sophia Yi, Lorenzo Pierini +4

Black hole spectroscopy is a clean and powerful tool to test gravity in the strong-field regime and to probe the nature of compact objects. Next-generation ground-based detectors,…