activity
19952026
most citedQuasi-Normal Modes of Stars and Black Holes

2.1k citations · 15.5k across the 182 of their papers we have counts for

collaborators

181 papers

gr-qc2026

Constraining the geometry of rotating black holes with eikonal QNMs

Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas

Quasinormal modes of black holes provide a central avenue for confronting general relativity with gravitational-wave observations from the ringdown stage of compact binary coalesce…

gr-qc2026

Tidally-enhanced resonances in extreme-mass-ratio inspirals: A tertiary path to chaos

Kyriakos Destounis, Takuya Katagiri, Sajal Mukherjee +1

Extreme-mass-ratio inspirals (EMRIs) provide a unique laboratory for probing strong-field gravity and complex relativistic dynamics. We study a tidally deformed EMRI composed of a…

gr-qc2026

Parametrized beyond-Teukolsky framework in the time domain

Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas +1

Modifications to General Relativity can significantly alter the perturbative response of black holes, leaving imprints on quasinormal-mode spectra, waveform amplitudes and phases,…

astro-ph.HE2026

Magnetorotational instabilities in solids: Application to neutron-star crusts

Arthur G. Suvorov, Thomas Celora, Kostas D. Kokkotas

The magnetorotational instability can generate strong, turbulent substructure within magnetized shear flows. The efficacy of the mechanism as a function of microphysical aspects of…

astro-ph.HE2026

Modeling X-ray reflection spectra from returning radiation: application to 4U 163047

Kostas Kourmpetis, Shafqat Riaz, Honghui Liu +6

Returning radiation is thought to play a key role in disk illumination of black hole X-ray binaries in the high-soft state, yet it has not been fully incorporated into XSPEC reflec…

gr-qc2026★ 1 cited

Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr

Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas +2

The accurate computation of quasinormal modes from rotating black holes beyond general relativity is crucial for testing fundamental physics with gravitational waves. In this study…