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Zenginoglu, Phys

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it
abstract

Black hole perturbation theory is typically studied on time surfaces that extend between the bifurcation sphere and spatial infinity. From a physical point of view, however, it may be favorable to employ time surfaces that extend between the future event horizon and future null infinity. This framework resolves problems regarding the representation of quasinormal mode eigenfunctions and the construction of short-ranged potentials for the perturbation equations in frequency domain.

citation-role summary

background 2

citation-polarity summary

fields

gr-qc 4

years

2026 1 2025 3

roles

background 2

polarities

background 2

representative citing papers

Exceptional Points and Resonance in Black Hole Ringdown

gr-qc · 2025-12-01 · conditional · novelty 7.0

An exceptional-point framework for black-hole ringdown characterizes resonances near avoided crossings, demonstrates enhanced mode contributions in the time domain, and identifies the EP frequency as the physically relevant observable.

Total absorption of tailored incoming signals by black holes

gr-qc · 2025-09-23 · unverdicted · novelty 7.0

Tailored temporal modulation of incoming signals enables complete absorption by black holes via excitation of complex-plane resonances, storing energy for later release through virtual absorption modes.

Black hole spectroscopy: from theory to experiment

gr-qc · 2025-05-29 · unverdicted · novelty 2.0

A review summarizing the state of the art in black hole quasinormal modes, ringdown waveform modeling, current LIGO-Virgo-KAGRA observations, and prospects for LISA and next-generation detectors.

citing papers explorer

Showing 4 of 4 citing papers.

  • Exceptional Points and Resonance in Black Hole Ringdown gr-qc · 2025-12-01 · conditional · none · ref 42 · internal anchor

    An exceptional-point framework for black-hole ringdown characterizes resonances near avoided crossings, demonstrates enhanced mode contributions in the time domain, and identifies the EP frequency as the physically relevant observable.

  • Total absorption of tailored incoming signals by black holes gr-qc · 2025-09-23 · unverdicted · none · ref 42 · internal anchor

    Tailored temporal modulation of incoming signals enables complete absorption by black holes via excitation of complex-plane resonances, storing energy for later release through virtual absorption modes.

  • Bilinear products and the orthogonality of quasinormal modes on hyperboloidal foliations gr-qc · 2026-04-14 · unverdicted · none · ref 43

    Bilinear products for black hole quasinormal modes on hyperboloidal foliations are divergent due to CPT transformations but can be regularized to define orthogonal modes and excitation coefficients.

  • Black hole spectroscopy: from theory to experiment gr-qc · 2025-05-29 · unverdicted · none · ref 292

    A review summarizing the state of the art in black hole quasinormal modes, ringdown waveform modeling, current LIGO-Virgo-KAGRA observations, and prospects for LISA and next-generation detectors.