Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field

Details Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field

1999-02-23

arxiv.org/abs/gr-qc/9902072v4

Phys.Rev.D61:024033,2000

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

20 pages

Scientific paper

10.1103/PhysRevD.61.024033

We present an analytic study of the mode-coupling phenomena for a scalar field propagating on a rotating Kerr background. Physically, this phenomena is caused by the dragging of reference frames, due to the black-hole (or star's) rotation. We find that different modes become mixed during the evolution and the asymptotic late-time tails are dominated by a mode which, in general, has an angular distribution different from the original one. We show that a rotating Kerr black hole becomes `bald' slower than a spherically-symmetric Schwarzschild black hole.

Affiliated with

Also associated with

No associations

Rating

Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field 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 Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-319543