11th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities

Session

Electronics/Software/Trigger

Jun 11, 2026, 1:30 PM

Schlosshotel Karlsruhe

29. Science Verification Analysis for Radio Neutrino Observatory in Greenland (RNO-G): Methods and Implementation

Zeynep Su Selcuk (DESY Zeuthen)

6/11/26, 1:30 PM

The Radio Neutrino Observatory in Greenland (RNO-G) aims to detect ultra-high-energy (UHE) neutrinos using radio technology. The detector array is planned to consist of 35 individual stations when finished and is currently under construction. As of March 2026, eight of these stations have already been commissioned with more to follow each year. To enable an efficient and effective installation...

7. The Data Acquisition System for the Radio Instrument of POEMMA Balloon with Radio (PBR)

Dr Alexander Novikov (University of Delaware)

6/11/26, 1:45 PM

POEMMA (Probe of Extreme Multimessenger Astrophysics) Balloon with Radio (PBR) is a balloon-borne experiment being prepared for launch in 2028 from Wanaka, New Zealand, with three key instruments: Fluorescence Camera (FC), Cherenkov Camera (CC), and a Radio Instrument (RI). This talk is focused on the RI consisting of two dual-polarized sinuous antennas with bandwidth of (60 – 500) MHz and...

8. Development of Readout Electronics of the IceCube-Gen2 Surface Array

Frederik Schmitt (KIT (IAP))

6/11/26, 2:00 PM

The IceCube Neutrino Observatory consists of two detector components: a cubic-kilometer in-ice neutrino detector and the IceTop surface array for high-energy cosmic rays. The proposed next-generation neutrino observatory, IceCube-Gen2, will increase the in-ice instrumented volume and add an additional in-ice radio detector for high-energy neutrinos. Furthermore, it will feature an entirely new...

1. Station-level neural-network trigger for radio detection of cosmic-ray air showers on FPGA

Vesselin Dimitrov (Center for Particle Physics Siegen, Department für Physik, Universität Siegen, Germany, and Peter Grünberg Institute - Integrated Computing Architectures (ICA | PGI-4), Forschungszentrum Jülich GmbH, Germany)

6/11/26, 2:15 PM

Radio detection of extensive air showers induced by ultra-high-energy cosmic rays provides crucial information on their origin, composition and energy. Radio arrays detect these events, but cosmic-ray signals are exceedingly rare compared to the overwhelming radio noise and RFI. Since storing all data is not feasible, a trigger system must decide in real time which data to record. FPGAs are a...

5. Enhancing the neutrino detection rate of in-ice radio detectors with neural-network-based triggers

René Reimann (TU Dortmund)

6/11/26, 2:30 PM

Radio detection of neutrinos remains the most promising technique for the detection of UHE neutrinos. Construction of large-scale radio-neutrino detectors, however, is limited by logistics; thus, optimization of the detector stations is the only way to enhance the science reach of future radio detectors. Improving the trigger efficiency also for faint signals is thus crucial. A complete...

21. What is new in NuRadioMC: Multilayer Analytic Ray-Tracing

Hannes Warnhofer (Deutsches Elektronen-Synchrotron DESY / Friedrich-Alexander-University Erlangen-Nuremberg)

6/11/26, 2:45 PM

NuRadioMC is a framework for the simulation of ultra-high-energy neutrino detectors that measure the radio signal emitted in neutrino-induced particle cascades. It is used in different radio neutrino experiments, such as RNO-G and is partly adopted by the cosmic-ray detectors LOFAR and SKA. The software enables end-to-end simulation of all relevant components starting with the neutrino...