Analytic structure of radiation boundary kernels for blackhole perturbations

Details Analytic structure of radiation boundary kernels for blackhole perturbations Analytic structure of radiation boundary kernels for blackhole perturbations

2005-07-29

arxiv.org/abs/gr-qc/0507140v1

J.Math.Phys. 46 (2005) 102503

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

revtex4, 14 pages, 12 figures, 3 tables

Scientific paper

10.1063/1.2073287

Exact outer boundary conditions for gravitational perturbations of the Schwarzschild metric feature integral convolution between a time-domain boundary kernel and each radiative mode of the perturbation. For both axial (Regge-Wheeler) and polar (Zerilli) perturbations, we study the Laplace transform of such kernels as an analytic function of (dimensionless) Laplace frequency. We present numerical evidence indicating that each such frequency-domain boundary kernel admits a "sum-of-poles" representation. Our work has been inspired by Alpert, Greengard, and Hagstrom's analysis of nonreflecting boundary conditions for the ordinary scalar wave equation.

Affiliated with

Also associated with

No associations

Rating

Analytic structure of radiation boundary kernels for blackhole perturbations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Analytic structure of radiation boundary kernels for blackhole perturbations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analytic structure of radiation boundary kernels for blackhole perturbations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-562485