Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark Matter
hep-ph, astro-ph.CO, hep-ex
Submitted: 2026-09-30
Updated: 2026-09-30
Comments: 27 pages, 3 figures, 4 tables
Code: https://github.com/Berkeley-Electroweak-Physics/Elastic
License: http://creativecommons.org/publicdomain/zero/1.0/
The gist: The LUX-ZEPLIN (LZ) experiment has recently reported a nuclear-recoil candidate at E R 248 keV.
Terminology
Abstract
The LUX-ZEPLIN (LZ) experiment has recently reported a nuclear-recoil candidate at E R 248 keV. We study two supersymmetric interpretations based on distinct neutralino couplings to the Z boson. In the elastic case, a bino- or singlino-like neutralino scatters through a diagonal axial Z coupling set by the Higgsino asymmetry X=N 13 2-N 14 squared rather than by the total Higgsino fraction. Since the spin-dependent blind spot does not coincide with the spin-independent one, Higgs-mediated scattering can be suppressed while retaining X about10-2. In the MSSM this favors low β, in tension with the observed Higgs mass for a few-TeV squark spectrum, a tension relieved by the tree-level quartic of the NMSSM. An explicit NMSSM benchmark with m χ 500 GeV and X 0.007, below current LZ limits, obtains its relic abundance from a singlet-like pseudoscalar resonance just above threshold, which also suppresses present-day annihilation. In the inelastic case, a pseudo-Dirac Higgsino scatters endothermically, with a splitting of a few hundred keV generated by gauginos at the PeV scale which can be lowered by opposite-sign bino-wino cancellation, or by weak singlino mixing; the minimal thermal realization is strongly constrained by solar-neutrino searches. The two mechanisms predict distinct recoil spectra away from the candidate.
Sources
- A Vector-Like Lepton Interpretation of the High-Energy Nuclear Recoil Candidate in LUX-ZEPLIN
- Inelastic Dark Matter
- The Effective Field Theory of Dark Matter Direct Detection
- Model-independent WIMP Scattering Responses and Event Rates: A Mathematica Package for Experimental Analysis
- Dark Matter at the Kinematic Edge: Interpreting the 248 keV LZ Nuclear-Recoil Candidate
- The Well-Tempered Neutralino
- The Next-to-Minimal Supersymmetric Standard Model
- Prospects and Blind Spots for Neutralino Dark Matter
- Blind Spots for neutralino Dark Matter in the MSSM with an intermediate m_A
- Blind spots for neutralino dark matter in the NMSSM
- Higgs Portals for Thermal Dark Matter - EFT Perspectives and the NMSSM -
- A relatively light, highly bino-like dark matter in the $Z_3$-symmetric NMSSM and recent LHC searches
- Electroweak Phase Transition in the $Z_3$-invariant NMSSM: Implications of LHC and Dark matter searches and prospects of detecting the gravitational waves
- Hunting ewinos and a light scalar of $Z_3$-NMSSM with a bino-like dark matter in top squark decays at the LHC
- Shedding Light on Dark Matter at the LHC with Machine Learning
- Dark Matter searches with photons at the LHC
- Higgsino Dark Matter in High-Scale Supersymmetry
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
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