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20022026
most citedInstability of the massive Klein-Gordon field on the Kerr spacetime

511 citations · 4.3k across the 78 of their papers we have counts for

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Showing 2014 · gr-qcShow all

6 papers · 2 filters

gr-qc2014★ 38 cited

Inferring black hole charge from backscattered electromagnetic radiation

Luís C. B. Crispino, Sam R. Dolan, Atsushi Higuchi +1

We compute the scattering cross section of Reissner-Nordström black holes for the case of an incident electromagnetic wave. We describe how scattering is affected by both the conve…

gr-qc2014★ 34 cited

Quasinormal modes and Regge poles of the canonical acoustic hole

Sam R. Dolan, Leandro A. Oliveira, Luis C. B. Crispino

We compute the quasinormal mode frequencies and Regge poles of the canonical acoustic hole (a black hole analogue), using three methods. First, we show how damped oscillations aris…

gr-qc2014★ 70 cited

Tidal invariants for compact binaries on quasi-circular orbits

Sam R. Dolan, Patrick Nolan, Adrian C. Ottewill +2

We extend the gravitational self-force approach to encompass `self-interaction' tidal effects for a compact body of mass on a quasi-circular orbit around a black hole of mass $…

gr-qc2014★ 92 cited

Gravitational Self-Force Correction to the Innermost Stable Circular Equatorial Orbit of a Kerr Black Hole

Soichiro Isoyama, Leor Barack, Sam R. Dolan +5

For a self-gravitating particle of mass μin orbit around a Kerr black hole of mass M >> μ, we compute the O(μ/M) shift in the frequency of the innermost stable circular equatorial…

gr-qc2014★ 75 cited

Absorption of a massive scalar field by a charged black hole

Carolina L. Benone, Ednilton S. de Oliveira, Sam R. Dolan +1

We calculate the absorption cross section of a massive neutral scalar field impinging upon a Reissner-Nordström black hole. First, we derive key approximations in the high- and low…

gr-qc2014★ 38 cited

Self-force via Green functions and worldline integration

Barry Wardell, Chad R. Galley, Anil Zenginoglu +3

A compact object moving in curved spacetime interacts with its own gravitational field. This leads to both dissipative and conservative corrections to the motion, which can be inte…