On the importance of cosmic-ray background in the Atomki anomaly
Abstract
We report Geant4-based simulations of cosmic-ray muon backgrounds in models reproducing the geometries of the five-arm and six-arm e+e- pair spectrometers operated by the Atomki group at Debrecen. Full detector geometries are implemented for both setups, including position-sensitive detectors and plastic scintillators. In both configurations, cosmic muons generating two-arm coincidences produce statistically significant excesses in the opening-angle distribution whose positions are determined by the discrete azimuthal arrangement of detector arms and the plastic scintillators dimensions: in the six-arm spectrometer a peak appears near 140 degrees when the scintillator energy sum is selected in the 8Be transition window (16-20 MeV) and is suppressed for energy-asymmetric pairs, while a distinct peak near 120 degrees emerges in the 4He window (18-22 MeV), with no comparable enhancement in the respective background energy region. These angles, asymmetry dependences, and background characteristics show behaviours similar to those reported by the Atomki group as evidence for a 17 MeV boson. For the five-arm setup, a 140-degree excess is also reproduced at 8Be energies, and normalizing internal pair conversion events and cosmic coincidences to typical Atomki running conditions yields a cosmic-to-IPC ratio above unity in the signal window, indicating that the cosmic background is a leading contribution to the event rate at the energies and angles of interest. While they do not settle the question of the origin of the Atomki excesses, these results highlight the critical importance of a robust cosmic-ray treatment in this type of measurements, and call for a detailed description of the beam-off studies supporting the search for anomalies in the opening-angle vs. energy-sum distribution around the signal region.
Related
- Radiative and Dalitz decays of Υ(1S) in the light of the ATOMKI X17 anomaly
- Domain Adaptation against Background Sculpting in Anomaly Detection at the LHC
- Optimization of multi-resolution observation strategies for cosmic microwave background experiments
- Joint measurements of thermal Sunyaev-Zel'dovich and cosmic infrared background cross-correlations with cosmic shear
- Quantum corrections to cosmic perturbations for a bouncing background
BibTeX
@misc{benmansour2026importance,
title = {{On the importance of cosmic-ray background in the Atomki anomaly}},
author = {Hicham Benmansour and Gianluigi Boca and Gianluca Cavoto and Marco Chiappini and Elia G. Grandoni and Luca Galli and Giovanni Gallucci and Angela Papa and Francesco Renga and Antoine Venturini and Cecilia Voena},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.18383},
eprint = {2609.18383},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.18383},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - On the importance of cosmic-ray background in the Atomki anomaly
AU - Hicham Benmansour
AU - Gianluigi Boca
AU - Gianluca Cavoto
AU - Marco Chiappini
AU - Elia G. Grandoni
AU - Luca Galli
AU - Giovanni Gallucci
AU - Angela Papa
AU - Francesco Renga
AU - Antoine Venturini
AU - Cecilia Voena
PY - 2026
DA - 2026/09/16
PB - arXiv
DO - 10.48550/arxiv.2609.18383
UR - https://arxiv.org/abs/2609.18383
AB - We report Geant4-based simulations of cosmic-ray muon backgrounds in models reproducing the geometries of the five-arm and six-arm e+e- pair spectrometers operated by the Atomki group at Debrecen. Full detector geometries are implemented for both setups, including position-sensitive detectors and plastic scintillators. In both configurations, cosmic muons generating two-arm coincidences produce statistically significant excesses in the opening-angle distribution whose positions are determined by the discrete azimuthal arrangement of detector arms and the plastic scintillators dimensions: in the six-arm spectrometer a peak appears near 140 degrees when the scintillator energy sum is selected in the 8Be transition window (16-20 MeV) and is suppressed for energy-asymmetric pairs, while a distinct peak near 120 degrees emerges in the 4He window (18-22 MeV), with no comparable enhancement in the respective background energy region. These angles, asymmetry dependences, and background characteristics show behaviours similar to those reported by the Atomki group as evidence for a 17 MeV boson. For the five-arm setup, a 140-degree excess is also reproduced at 8Be energies, and normalizing internal pair conversion events and cosmic coincidences to typical Atomki running conditions yields a cosmic-to-IPC ratio above unity in the signal window, indicating that the cosmic background is a leading contribution to the event rate at the energies and angles of interest. While they do not settle the question of the origin of the Atomki excesses, these results highlight the critical importance of a robust cosmic-ray treatment in this type of measurements, and call for a detailed description of the beam-off studies supporting the search for anomalies in the opening-angle vs. energy-sum distribution around the signal region.
ER -