most citedGW250114 reveals black hole horizon signatures

1 citations · 1 across the 4 of their papers we have counts for

collaborators

6 papers

gr-qc2026

Accounting for detector calibration uncertainty in black-hole ringdown analysis

Rowina S. Nathan, Shingo Hido, Neil Lu +3

Detector calibration systematics can bias measurements of a remnant black hole's mass and spin, producing spurious evidence against general relativity if unaccounted for. The ringd…

gr-qc2026

A semicoherent resampling method for long-transient gravitational wave searches with applications to subsolar-mass primordial black-hole binaries

Neil Lu, Cristiano Palomba, Ornella J. Piccinni +1

Resampling removes the modeled phase evolution of a frequency-evolving signal, transforming it into a monochromatic one. We introduce a novel implementation for long-transient grav…

gr-qc2026

From driven oscillations to free ringdown: a particle plunging into Kerr

Colin Weller, Andrew Laeuger, Fulin Li +5

We show that a ringdown waveform can admit a constant-coefficient quasinormal-mode (QNM) representation while its individual QNM-pole contributions remain driven. To establish this…

gr-qc2026

Complex frequency evolution of direct waves from binary black hole mergers

Ling Sun, Sizheng Ma, Patrick P. Chen +3

While no signal originating at a black hole's event horizon can reach future null infinity, information about the horizon and its immediate vicinity can be encoded in asymptotic pr…

gr-qc2025★ 1 cited

GW250114 reveals black hole horizon signatures

Neil Lu, Sizheng Ma, Ornella J. Piccinni +2

The horizon of a black hole, the "surface of no return", is characterized by its rotation frequency and surface gravity . A striking signature is that any infalling object…

gr-qc2025

Statistical identification of ringdown modes with rational filters

Neil Lu, Sizheng Ma, Ornella J. Piccinni +2

Measuring quasinormal modes (QNMs) during the ringdown phase of binary black hole coalescences provides key insights into merger dynamics and enables tests of the no-hair theorem.…