Abstract
The low flux of the ultra-high energy cosmic rays (UHECR) at the highest
energies provides a challenge to answer the long standing question about
their origin and nature. A significant increase in the number of
detected UHECR is expected to be achieved by employing Earth''s moon as
detector, and search for short radio pulses that are emitted when a
particle interacts in the lunar rock. Observation of these short pulses
with current and future radio telescopes also allows to search for the
even lower fluxes of neutrinos with energies above 1022 eV,
that are predicted in certain Grand-Unifying-Theories (GUTs), and e.g.
models for super-heavy dark matter (SHDM). In this contribution we
present the initial design for such a search with the LOFAR radio
telescope.
| Original language | English |
|---|---|
| Title of host publication | 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities |
| Subtitle of host publication | ARENA 2016 |
| Publisher | EPJ Web of Conferences |
| Number of pages | 4 |
| Volume | 135 |
| DOIs | |
| Publication status | Published - 15-Mar-2017 |
| Event | 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities - Groningen, Netherlands Duration: 7-Jun-2016 → 10-Jun-2016 https://www.kvi.nl/~scholten/ARENA/WebSite/default.htm |
Conference
| Conference | 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities |
|---|---|
| Abbreviated title | ARENA 2016 |
| Country/Territory | Netherlands |
| City | Groningen |
| Period | 07/06/2016 → 10/06/2016 |
| Internet address |