Gravitational energy loss in high energy particle collisions: ultrarelativistic plunge into a multidimensional black hole

Details Gravitational energy loss in high energy particle collisions: ultrarelativistic plunge into a multidimensional black hole Gravitational energy loss in high energy particle collisions: ultrarelativistic plunge into a multidimensional black hole

2003-09-20

arxiv.org/abs/hep-th/0309203v2

Phys.Rev.D69:124011,2004

Physics

High Energy Physics

High Energy Physics - Theory

18 pages, 4 figures. Minor changes to match version accepted by PRD

Scientific paper

10.1103/PhysRevD.69.124011

We investigate the gravitational energy emission of an ultrarelativistic particle radially falling into a D-dimensional black hole. We numerically integrate the equations describing black hole gravitational perturbations and obtain energy spectra, total energy and angular distribution of the emitted gravitational radiation. The black hole quasinormal modes for scalar, vector, and tensor perturbations are computed in the WKB approximation. We discuss our results in the context of black hole production at the TeV scale.

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