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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.
| Verfasserangaben: | Benjamin KochORCiDGND, Hans-Joachim Drescher, Marcus BleicherORCiDGND |
|---|---|
| URN: | urn:nbn:de:hebis:30-26319 |
| Dokumentart: | Preprint |
| Sprache: | Englisch |
| Datum der Veröffentlichung (online): | 09.05.2006 |
| Jahr der Erstveröffentlichung: | 2006 |
| Veröffentlichende Institution: | Universitätsbibliothek Johann Christian Senckenberg |
| Datum der Freischaltung: | 09.05.2006 |
| Freies Schlagwort / Tag: | ADD; UHECR; cosmic rays; extra dimension; gravitational radiation |
| Quelle: | http://arxiv.org/abs/astro-ph/0602164 ; preprint submitted to Elsevier Science |
| HeBIS-PPN: | 190704608 |
| Institute: | Physik / Physik |
| DDC-Klassifikation: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
| Lizenz (Deutsch): |  Deutsches Urheberrecht |
