papers

Publications (24)

astro-ph.IM2024

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2024)

Rafael Alves Batista, Aurélien Benoit-Lévy, Teresa Bister +121

This is an index of the contributions by the Giant Radio Array for Neutrino Detection (GRAND) Collaboration to the 10th International Workshop on Acoustic and Radio EeV Neutrino De…

astro-ph.IM2021

A reconstruction procedure for near horizon extensive air showers based on radio signals

Valentin Decoene, Olivier Martineau-Huynh, Matìas Tueros +1

Very inclined extensive air showers (EAS), with both down-going and up-going trajectories, are particularly targeted by the next generation of extended radio arrays, such as GRAND.…

astro-ph.IM2025

Reconstruction of inclined cosmic-ray properties with GRAND data

Marion Guelfand, Pauline Fritsch, Valentin Decoene +2

Radio-detection is now an established technique for studying ultra-high-energy (UHE) cosmic rays with energies exceeding eV. The next generation of radio experiments…

astro-ph.IM2020

Radio-detection of neutrino-induced air showers: the influence of topography

Valentin Decoene, Nicolas Renault-Tinacci, Olivier Martineau-Huynh +6

Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This…

astro-ph.IM2024

Targeting 100-PeV tau neutrino detection with an array of phased and high-gain reconstruction antennas

Stephanie Wissel, Andrew Zeolla, Cosmin Deaconu +20

Neutrinos at ultrahigh energies can originate both from interactions of cosmic rays at their acceleration sites and through cosmic-ray interactions as they propagate through the un…

astro-ph.HE2023

Review of Neutrino Experiments Searching for Astrophysical Neutrinos

Valentin Decoene

Over the last two decades, we have intensified our search for a ghost particle, with the hope that it would provide us with information on the darkest places of our Universe. This…

astro-ph.IM2019

Radio Morphing: towards a fast computation of the radio signal from air showers

Anne Zilles, Olivier Martineau-Huynh, Kumiko Kotera +6

Over the last years, radio detection has matured to become a competitive method for the detection of air showers. Arrays of thousands of antennas are now envisioned for the detecti…

astro-ph.HE2024

Reconstruction of highly inclined extensive air showers in GRAND

Oscar Macias, Aurélien Benoit-Lévy, Valentin Decoene +8

The Giant Radio Array for Neutrino Detection (GRAND) aims to detect highly inclined extensive air showers (EAS) with down-going and up-going trajectories. Several working groups in…

astro-ph.HE2022

Overview of radio experiments for UHE cosmic particles detection

Simon Chiche, Valentin Decoene

Radio-detection is a mature technique that has gained large momentum over the past decades. Its physical detection principle is mainly driven by the electromagnetic part of the sho…

astro-ph.IM2026

Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes

GRAND Collaboration, Jaime Álvarez-Muniz, Rafael Alves Batista +118

The Giant Radio Array for Neutrino Detection (GRAND) is a proposed multi-messenger observatory of Ultra-High-Energy (UHE) particles of cosmic origin. Its main goal is to find the l…

astro-ph.IM2024

GRANDlib: A simulation pipeline for the Giant Radio Array for Neutrino Detection (GRAND)

GRAND Collaboration, Rafael Alves Batista, Aurélien Benoit-Lévy +112

The operation of upcoming ultra-high-energy cosmic-ray, gamma-ray, and neutrino radio-detection experiments, like the Giant Radio Array for Neutrino Detection (GRAND), poses signif…

astro-ph.HE2025

Analytical description of the radio Cherenkov cone

Valentin Decoene, Marion Guelfand, Matìas Tueros

Radio emissions from extensive air showers (EAS) provide a valuable tool for detecting ultra-high-energy (UHE) astroparticles. In this context, several radio arrays focus on detect…

astro-ph.HE2025

Reconstruction of inclined extensive air showers using radio signals: from arrival times and amplitudes to direction and energy

Marion Guelfand, Valentin Decoene, Olivier Martineau-Huynh +4

Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above eV. The next-generation of radio experiments…

astro-ph.IM2025

The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project

Kumiko Kotera, Ingo Allekotte, Jaime Alvarez-Muñiz +10

Measuring ultra-high energy neutrinos, with energies above eV, is the next frontier of the emerging multi-messenger era. Their detection requires building a large-scale d…

hep-ph2022

High-Energy and Ultra-High-Energy Neutrinos

Markus Ackermann, Sanjib K. Agarwalla, Jaime Alvarez-Muñiz +43

Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, h…

astro-ph.HE2020

Fast radio burst repeaters produced via Kozai-Lidov feeding of neutron stars in binary systems

Valentin Decoene, Kumiko Kotera, Joseph Silk

Neutron stars are likely surrounded by gas, debris, and asteroid belts. Kozai-Lidov perturbations, induced by a distant, but gravitationally bound companion, can trigger the infall…

astro-ph.IM2025

Optimizing HERON for 100 PeV Neutrino Detection

Andrew Zeolla, Ingo Allekotte, Jaime Alvarez-Muñiz +10

The Hybrid Elevated Radio Observatory for Neutrinos (HERON) is designed to target the astrophysical flux of Earth-skimming tau neutrinos at 100 PeV. HERON consists of multiple comp…

hep-ex2024

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)

GRAND Collaboration, Rafael Alves Batista, Aurélien Benoit-Lévy +96

The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses la…

astro-ph.IM2022

Radio wavefront of very inclined extensive air-showers: a simulation study for extended and sparse radio arrays

Valentin Decoene, Olivier Martineau-Huynh, Matias Tueros

Radio-detection is becoming an established technique for the detection of air showers induced by cosmic particles. This is in particular true at the highest energies, where very la…

astro-ph.IM2019

GRANDProto300: a pathfinder with richastroparticle and radio-astronomy science case

Valentin Decoene

The GRANDProto300 (GP300) experiment is the first stage of the Giant Radio Array for Neutrino Detection (GRAND) project. It will be deployed between 2020 and 2021 in a radio-quiet…

astro-ph.HE2020

High-energy neutrinos from fallback accretion of binary neutron star merger remnants

Valentin Decoene, Claire Guépin, Ke Fang +2

Following the coalescence of binary neutron stars, debris from the merger which remains marginally bound to the central compact remnant will fallback at late times, feeding a susta…

hep-ph2022

Tau Neutrinos in the Next Decade: from GeV to EeV

Roshan Mammen Abraham, Jaime Alvarez-Muñiz, Carlos A. Argüelles +63

Tau neutrinos are the least studied particle in the Standard Model. This whitepaper discusses the current and expected upcoming status of tau neutrino physics with attention to the…

astro-ph.HE2019

The Giant Radio Array for Neutrino Detection (GRAND): Science and Design

GRAND Collaboration, Jaime Alvarez-Muniz, Rafael Alves Batista +48

The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10^8 GeV. Its goal is…

astro-ph.IM2025

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC 2025)

Jaime Álvarez-Muñiz, Rafael Alves Batista, Aurélien Benoit-Lévy +133

The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses la…