Gravitational Radiation from Ultra High Energy Cosmic Rays in Models with Large Extra Dimensions

Simple item page
dc.creatorKoch, Ben
dc.creatorDrescher, Hans-Joachim
dc.creatorBleicher, Marcus
dc.date2006-02-07
dc.date.accessioned2026-07-07T11:03:57Z
dc.date.available2026-07-07T11:03:57Z
dc.descriptionThe effects of classical gravitational radiation in models with large extra dimensions are investigated for ultra high energy cosmic rays (CRs). The cross sections are implemented into a simulation package (SENECA) for high energy hadron induced CR air showers. We predict that gravitational radiation from quasi-elastic scattering could be observed at incident CR energies above $10^9$ GeV for a setting with more than two extra dimensions. It is further shown that this gravitational energy loss can alter the energy reconstruction for CR energies $E_{\rm CR}\ge 5\cdot 10^9$ GeV.
dc.identifierhttps://arxiv.org/abs/astro-ph/0602164
dc.identifierhttp://arxiv.org/abs/astro-ph/0602164
dc.identifierAstropart.Phys.25:291-297,2006
dc.identifierdoi:10.1016/j.astropartphys.2006.02.007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188722
dc.subjectAstrophysics
dc.titleGravitational Radiation from Ultra High Energy Cosmic Rays in Models with Large Extra Dimensions
dc.typetext

Files

Collections

arXiv