EPJ Web Conf.
Volume 216, 20198th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2018)
|Number of page(s)||3|
|Section||Future and Perspectives|
|Published online||24 September 2019|
Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR
Astrophysical Institute, Vrije Universiteit Brussel, Pleinlaan 2, 1050, Brussels, Belgium
2 Department of Astrophysics/IMAPP, Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
3 NIKHEF, Science Park Amsterdam, 1098 XG, Amsterdam, The Netherlands
4 Netherlands Institute of Radio Astronomy (ASTRON), Postbus 2, 7990 AA, Dwingeloo, The Netherlands
5 KVI-CART, University Groningen, P.O. Box 72, 9700 AB, Groningen
6 Department of Physics and Astronomy, University of California Irvine, 92697-4575, Irvine, CA, USA
7 Department of Astrophysical Sciences, Princeton University, Princeton,NJ, 08544, USA
8 Interuniversity Institute for High-Energy, Vrije Universiteit Brussel, Pleinlaan 2, 1050, Brussels, Belgium
9 Department of Physics and Electrical Engineering, Linnéuniversitetet, 35195, Växjö, Sweden
★ e-mail: firstname.lastname@example.org; This work is funded by ERC grant 640130 and DFG grant WI 4946/1-1
Published online: 24 September 2019
The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth’s moon as a detector that is read out using existing Earth-bound radio telescopes by searching for the radio pulses emitted by the particle shower in the lunar rock. In this contribution we will report on the properties of a corresponding detection mode currently under development for the LOFAR Radio telescope.
© The Authors, published by EDP Sciences, 2019
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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