Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole

Details Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole

2001-05-17

arxiv.org/abs/gr-qc/0105056v1

Phys.Rev. D64 (2001) 044024

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, 4 figures, to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.64.044024

We investigate the late-time tails of self-interacting (massive) scalar fields in the spacetime of dilaton black hole. Following the no hair theorem we examine the mechanism by which self-interacting scalar hair decay. We revealed that the intermediate asymptotic behavior of the considered field perturbations is dominated by an oscillatory inverse power-law decaying tail. The numerical simulations showed that at the very late-time massive self-interacting scalar hair decayed slower than any power law.

Affiliated with

Also associated with

No associations

Rating

Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole 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 Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-184632