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20212026
most citedDisks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms

115 citations · 229 across the 18 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

gr-qc2025

Gravitational Atom Spectroscopy

Matteo Della Rocca, Thomas F. M. Spieksma, Francisco Duque +2

Black holes in our Universe are rarely truly isolated, being instead embedded in astrophysical environments such as plasma or dark matter. A particularly intriguing possibility is…

gr-qc2025

Exploring Black Hole Environments

Thomas F. M. Spieksma

The past decade has transformed our ability to observe the Universe. Via gravitational waves, merging black holes and neutron stars can now be directly detected, offering unprecede…

gr-qc2025

Total absorption of tailored incoming signals by black holes

Furkan Tuncer, Vitor Cardoso, Rodrigo Panosso Macedo +1

We uncover a new class of phenomena in gravitational physics, whereby resonances in the complex plane can be excited via tailored time-dependent scattering. We show that specific f…

astro-ph.GA2025★ 6 cited

In the grip of the disk: dragging the companion through an AGN

Thomas F. M. Spieksma, Enrico Cannizzaro

Active galactic nuclei (AGN) have been proposed as environments that can facilitate the capture of extreme-mass-ratio binaries and accelerate their inspiral beyond the rate expecte…

hep-ph2025

Axion dissipation in conductive media and neutron star superradiance

Thomas F. M. Spieksma, Enrico Cannizzaro

In axion electrodynamics, magnetic fields enable axion-photon mixing. Recent proposals suggest that rotating, conductive plasmas in neutron star magnetospheres could trigger axion…

gr-qc2025★ 1 cited

Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr

Conor Dyson, Thomas F. M. Spieksma, Richard Brito +2

Future gravitational wave observatories open a unique avenue to study the environments surrounding black holes. Intermediate or extreme mass ratio inspirals will spend thousands to…