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Optimized trigger for ultra-high-energy cosmic-ray and neutrino observations with the low frequency radio array
Affiliation:a Kernfysisch Versneller Instituut, University of Groningen, 9747 AA Groningen, The Netherlands
b Vrije Universiteit Brussel, Dienst ELEM, B-1050 Brussels, Belgium
c Department of Physics, University of Alberta, Edmonton, AB, Canada T6G 2G7
d Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
e Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo, The Netherlands
f School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK
g Center for Astrophysics, Harvard University, USA
h Kapteyn Astronomical Institute, PO Box 800, 9700 AV Groningen, The Netherlands
i Institute for Astronomy, University of Edinburgh, Royal Observatory of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK
j Jacobs University Bremen, Campus Ring 1, 28759 Bremen, Germany
k Department of Astrophysics, IMAPP, Radboud University Nijmegen, 6500 GL Nijmegen, The Netherlands
l Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
m Mt Stromlo Observatory, Research School of Astronomy and Astrophysics, Australian National University, Weston, ACT 2611, Australia
n Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, 85741 Garching, Germany
o Astronomisches Institut der Ruhr-Universitaet Bochum, Universitaetsstrae 150, 44780 Bochum, Germany
p Thueringer Landessternwarte, Sternwarte 5, D-07778 Tautenburg, Germany
q Laboratoire de Physique et Chimie de l'Environnement et de l'Espace 3A, Avenue de la Recherche Scientifique 45071 Orleans cedex 2, France
r CIT, University of Groningen, The Netherlands
s Centre de Recherche Astrophysique de Lyon, Observatoire de Lyon, 9 av Charles André, 69561 Saint Genis Laval Cedex, France
t Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
u Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
v Astrophysikalisches Institut Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
w Argelander-Institute for Astronomy, University of Bonn, Auf dem Huegel 69, 53121 Bonn, Germany
Abstract:When an ultra-high energy neutrino or cosmic-ray strikes the Lunar surface a radio-frequency pulse is emitted. We plan to use the LOFAR radio telescope to detect these pulses. In this work we propose an efficient trigger implementation for LOFAR optimized for the observation of short radio pulses.
Keywords:Ultra-high energy cosmic rays   Ultra-high energy neutrinos   Lunar radio detection   Nano-second pulse detection   LOFAR   Frequency filter detection
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