Black Hole--Scalar Field Interactions in Spherical Symmetry

Details Black Hole--Scalar Field Interactions in Spherical Symmetry Black Hole--Scalar Field Interactions in Spherical Symmetry

1996-07-15

arxiv.org/abs/gr-qc/9607034v1

Phys.Rev.D54:4929-4943,1996

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages, 26 figures, RevTex, to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.54.4929

We examine the interactions of a black hole with a massless scalar field using a coordinate system which extends ingoing Eddington-Finkelstein coordinates to dynamic spherically symmetric-spacetimes. We avoid problems with the singularity by excising the region of the black hole interior to the apparent horizon. We use a second-order finite difference scheme to solve the equations. The resulting program is stable and convergent and will run forever without problems. We are able to observe quasi-normal ringing and power-law tails as well an interesting nonlinear feature.

Affiliated with

Also associated with

No associations

Rating

Black Hole--Scalar Field Interactions in Spherical Symmetry 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 Black Hole--Scalar Field Interactions in Spherical Symmetry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Black Hole--Scalar Field Interactions in Spherical Symmetry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-577989