Probing Light Dark Particles in Neutrino Scattering Experiments
Ruofei Feng, Shao-Feng Ge, Yongchao Zhang
TL;DR
This work develops a model‑independent EFT framework for neutrino–dark fermion absorption via five Lorentz structures, and applies it to neutrino scattering experiments. By analyzing COHERENT and CONUS+ CEνNS data, it derives hadronic (nucleon) operator limits Λ_{i,N}, finding them weaker than current LHC and SN1987A constraints, with notable isospin‑dependent suppression for IV vector interactions. The study then examines DUNE near‑detector prospects for leptonic (electron) couplings, showing sensitivity to Λ_{i,e} up to ~1 TeV for mχ up to ~100 MeV, surpassing CHARM II and LEP in several channels. The results highlight complementarity between CEνNS and ν–e scattering probes and illustrate how near‑term and future facilities, along with high‑energy colliders, map different regions of the parameter space for neutrino–dark sector interactions. Overall, DUNE ND emerges as a key platform for testing heavy‑mediator EFTs of ν–χ interactions with electrons, while current CEνNS data provide important cross‑checks against non‑hadronic channels and guide interpretations of collider and astrophysical bounds.
Abstract
In this work we investigate the production of a dark fermionic particle $χ$ in the neutrino scattering experiments. In the framework of effective field theory, such process can be induced by the effective four-fermion interactions involving neutrinos, the dark particle $χ$ and standard model particles. In particular, we examine the constraints on the effective couplings from the neutrinos scattering off nuclei in the COHERENT and CONUS+ experiments as well as the prospects at the DUNE near detector from neutrino-electron scattering. It turns out the current COHERENT and CONUS+ constraints on the cutoff scales are less stringent than those from the existing Large Hadron Collider data. However, the DUNE near detector could probe the cutoff scales beyond the existing CHARM II and LEP limits up to roughly 1 TeV, for the dark particle mass up to roughly 50 MeV.
