Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry

Details Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry

2002-01-21

arxiv.org/abs/hep-th/0201162v2

Phys.Rev. D65 (2002) 104033

Physics

High Energy Physics

High Energy Physics - Theory

13 pages, 6 figures, published version. References added

Scientific paper

10.1103/PhysRevD.65.104033

We present a complete relativistic analysis for the scalar radiation emitted by a particle in circular orbit around a Schwarzschild-anti-de Sitter black hole. If the black hole is large, then the radiation is concentrated in narrow angles- high multipolar distribution- i.e., the radiation is synchrotronic. However, small black holes exhibit a totally different behavior: in the small black hole regime, the radiation is concentrated in low multipoles. There is a transition mass at $M=0.427 R$, where $R$ is the AdS radius. This behavior is new, it is not present in asymptotically flat spacetimes.

Affiliated with

Also associated with

No associations

Rating

Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry 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 Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Scalar Synchrotron Radiation in the Schwarzschild-anti-de Sitter Geometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-12537