Drell-Yan Production of New Particles at Fixed-Target Experiments: Heavy Neutral Lepton as a Case Study
Francis M. Burk, P. S. Bhupal Dev, Bhaskar Dutta, Tao Han, Aparajitha Karthikeyan, Doojin Kim
TL;DR
The paper investigates how Drell–Yan production from deep inelastic scattering can illuminate light BSM physics at fixed-target experiments, using heavy neutral leptons (HNLs) produced via a light vector mediator $Z'$ with $m_{Z'}\in[2,20]$ GeV. Employing PDFs and a narrow-width resonance framework, the authors compute $pp\to Z'\to NN$ cross sections and project detectable yields for SBND, DarkQuest, DUNE ND, and SHiP, focusing on HNL decays $N\to \nu\pi^0$ and $N\to \nu e^+e^-$. They demonstrate that the Drell–Yan channel yields more energetic final states than meson-decay production, enabling robust background rejection, and they report 90% CL sensitivities on the HNL mixing $|U_\tau|$ and $U(1)_X$ gauge couplings $g_X$ across $U(1)_{B-L}$, $U(1)_{B-3L_τ}$, and $U(1)_B$ models, including reach to the Type-I seesaw band for DUNE ND and SHiP. The results show substantial improvement over current bounds and indicate that fixed-target experiments can comprehensively probe light dark sector scenarios, with potential extensions to other light mediators and dark matter models.
Abstract
We demonstrate the sensitivity of Drell-Yan production processes from deep inelastic scattering in searches for beyond-the-Standard Model (BSM) physics at fixed-target or beam-bump experiments. We take heavy neutral leptons (HNLs) as a case study, produced from the decay of a light vector boson mediator with mass in the range of $2-20$ GeV, which itself is generated via the Drell-Yan process. The produced HNLs subsequently decay into Standard Model final states. We consider several current and future experiments, including SBND, DarkQuest, DUNE Near Detector (ND), and SHiP. Utilizing $νπ^0$ and $νe^+e^-$ final states from HNL decays, we find that the Drell-Yan mechanism provides important contributions and significantly enhances the HNL search sensitivity, owing to the production of energetic final-state particles that are more readily detectable over the expected backgrounds. We find that at $90\%$ C.L. sensitivity, for gauge couplings $g_{X} \sim 10^{-2}\ (10^{-3})$ and kinematically accessible mass range, SBND and DarkQuest can probe the HNL flavor mixing $|U_{\ell}| \sim 3\times 10^{-4}\ (10^{-3})$, whereas DUNE ND and SHiP may extend the sensitivity down to the Type-I Seesaw prediction of $|U_{\ell}| \sim 10^{-5}$. Finally, for our chosen benchmark $|U_{\ell}| = 10^{-3}$ outside of the current experimental constraints, with a fixed mass ratio $m_{Z'}/m_N = 2.1$, and working within the $U(1)_{B-L}$, $U(1)_{B-3L_τ}$, and $U(1)_{B}$ parameter spaces, we find that both SBND and DarkQuest can probe $g_{X} \sim 10^{-3}$, DUNE ND can reach $g_{X} \sim 10^{-4}$, and SHiP can probe down to $g_{X}\sim 5\times 10^{-6}$. Our approach provides a powerful new technique to study HNL production at future fixed-target experiments and can readily be extended to other light BSM particle production within a broader class of dark sector models.
