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

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

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

Keywords

High Energy Physics - Theory, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/197521

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/hep-th/0309203
 http://arxiv.org/abs/hep-th/0309203
 Phys.Rev.D69:124011,2004
 doi:10.1103/PhysRevD.69.124011

Collections

arXiv