Complementary Search of Fermionic Absorption Operators at Hadron Collider and Direct Detection Experiments
Kai Ma, Shao-Feng Ge, Lin-Yun He, Ning Zhou
TL;DR
This work formulates fermionic dark sector absorption interactions via a quark–neutrino–chi EFT with five leading Lorentz structures and studies their collider and direct-detection signatures. By evaluating mono-photon, mono-jet, and mono-Z channels at the LHC, the authors extract current and projected limits on the operator scales $\Lambda_i$, finding that mono-Z leptonic decays often provide the strongest collider constraints, reaching $\Lambda \sim \mathcal{O}(\text{TeV})$ for light $m_\chi$. They then connect these collider probes to nuclear-target absorption on nuclei, deriving SI and SD scattering rates and comparing with DD experiments; light targets like Borexino yield especially strong SD bounds, while heavy-nucleus detectors excel for SI bounds depending on the operator. Overall, the paper demonstrates a complementary landscape where collider searches constrain DS absorption operators in regions where direct-detection and neutrino experiments are less sensitive, and vice versa, highlighting the tensor operator as a particularly rich case with competing SI and SD contributions. The results guide future explorations at HL-LHC/HE-LHC and inform cross-experimental strategies for probing light dark-sector fermions via absorption mechanisms.
Abstract
Instead of the energy recoil signal at direct detection experiments, dark fermion appears as missing energy at hadron colliders. For a fermionc dark sector particle that coupled with quarks and neutrino via absorption operators, its production at collider is accompanied by an invisible neutrino. We study in details the mono-$X$ (photon, jet, and $Z$) productions at the Large Hadron Collider (LHC). We start from the quark-level absorption operators to make easy comparison between the collider and direct detection experiments. In other words, we study the model-independent constraints on a dark fermion with absorption operator. In addition, the interplay and comparison with the possible detection at the neutrino experiments, especially Borexino, is also briefly discussed. We find that light nuclear target can provide the stronger constraints on both spin-dependent and spin-independent absorption operators.
