Applying black hole perturbation theory to numerically generated spacetimes

Details Applying black hole perturbation theory to numerically generated spacetimes Applying black hole perturbation theory to numerically generated spacetimes

1995-08-29

arxiv.org/abs/gr-qc/9508059v1

Phys.Rev. D53 (1996) 1963-1971

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages, revtex3.0, 5 figures

Scientific paper

10.1103/PhysRevD.53.1963

Nonspherical perturbation theory has been necessary to understand the meaning of radiation in spacetimes generated through fully nonlinear numerical relativity. Recently, perturbation techniques have been found to be successful for the time evolution of initial data found by nonlinear methods. Anticipating that such an approach will prove useful in a variety of problems, we give here both the practical steps, and a discussion of the underlying theory, for taking numerically generated data on an initial hypersurface as initial value data and extracting data that can be considered to be nonspherical perturbations.

Affiliated with

Also associated with

No associations

Rating

Applying black hole perturbation theory to numerically generated spacetimes 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 Applying black hole perturbation theory to numerically generated spacetimes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Applying black hole perturbation theory to numerically generated spacetimes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-437796