Gravitational radiation from ultra high energy cosmic rays in models with large extra dimensions

  • The 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_CR > 5 10^9 GeV.

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Metadaten
Author:Benjamin KochORCiDGND, Hans-Joachim Drescher, Marcus BleicherORCiDGND
URN:urn:nbn:de:hebis:30-26319
Document Type:Preprint
Language:English
Date of Publication (online):2006/05/09
Year of first Publication:2006
Publishing Institution:Universit├Ątsbibliothek Johann Christian Senckenberg
Release Date:2006/05/09
Tag:ADD; UHECR; cosmic rays; extra dimension; gravitational radiation
Source:http://arxiv.org/abs/astro-ph/0602164 ; preprint submitted to Elsevier Science
HeBIS-PPN:190704608
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Licence (German):License LogoDeutsches Urheberrecht