Sensitivity to sub-GeV dark matter in forthcoming spallation-source neutrino experiments
D. Aristizabal Sierra, V. De Romeri, D. K. Papoulias, G. Sanchez Garcia

TL;DR
This paper explores how upcoming neutrino experiments at spallation sources can detect sub-GeV dark matter via neutral pion decays, offering new avenues for probing elusive dark matter models beyond traditional methods.
Contribution
It introduces a novel sensitivity analysis of future neutrino detectors to light dark matter produced in pion decays, comparing simulation approaches and highlighting potential for new discoveries.
Findings
Upcoming neutrino detectors can test unexplored dark matter parameter space.
GEANT4 and Sandford-Wang approaches yield consistent predictions.
Facilities like ESS, J-PARC, and CSNS can enhance the search for secluded sectors.
Abstract
Sub-GeV thermal dark matter weakly interacting with the Standard Model through vector-portal mediators provides a well-motivated and predictive framework that remains challenging to probe with conventional direct detection experiments. Motivated by the rapid development of neutrino facilities based on spallation neutron sources, we study the sensitivity of future coherent elastic neutrino-nucleus scattering experiments to light dark matter produced in neutral pion decays. We consider scalar dark matter interactions mediated by two different vector portals, a generic dark photon and a baryophilic vector mediator. The neutral pion yield is calculated through a GEANT4 simulation and the results are compared with those obtained with the Sandford-Wang parametrization. We show that predictions based on either approach do not produce significant differences. Our results demonstrate that…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Particle physics theoretical and experimental studies
