activity
20042026
most citedEigenvalues and eigenfunctions of spin-weighted spheroidal harmonics in four and higher dimensions

337 citations · 1.8k across the 50 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

gr-qc2016★ 18 cited

High-order tail in Kerr spacetime

Marc Casals, Chris Kavanagh, Adrian C. Ottewill

We investigate the late-time tail of the retarded Green function for the dynamics of a linear field perturbation of Kerr spacetime. We develop an analytical formalism for obtaining…

gr-qc2016★ 44 cited

Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities

Marc Casals, Alessandro Fabbri, Cristián Martínez +1

We analytically investigate backreaction by a quantum scalar field on two rotating Bañados-Teitelboim-Zanelli (BTZ) geometries: that of a black hole and that of a naked singularity…

gr-qc2016★ 60 cited

Horizon Instability of Extremal Kerr Black Holes: Nonaxisymmetric Modes and Enhanced Growth Rate

Marc Casals, Samuel E. Gralla, Peter Zimmerman

We show that the horizon instability of the extremal Kerr black hole is associated with a singular branch point in the Green function at the superradiant bound frequency. We study…

gr-qc2016★ 4 cited

Spin-1 Quasi-normal Frequencies in Schwarzschild space-time for Large Overtone Number

Marc Casals, Adrian C. Ottewill

We analytically investigate the spin-1 quasinormal mode frequencies of Schwarzschild black hole space-time. We formally determine these frequencies to arbitrary order as an expansi…

gr-qc2016★ 8 cited

Global Hadamard form for the Green Function in Schwarzschild space-time

Marc Casals, Brien Nolan

The retarded Green function of a wave equation on a 4-dimensional curved background spacetime is a (generalized) function of two spacetime points and diverges when these are connec…

hep-th2016★ 33 cited

Quantum dress for a naked singularity

Marc Casals, Alessandro Fabbri, Cristián Martínez +1

We investigate semiclassical backreaction on a conical naked singularity space-time with a negative cosmological constant in (2+1)-dimensions. In particular, we calculate the renor…