Higgsino dark matter compatible with the LUX-ZEPLIN high-energy nuclear-recoil event and IceCube constraints
hep-ph, astro-ph.CO, hep-th
Submitted: 2026-10-02
Updated: 2026-10-02
Sources
- Final model independent result of DAMA/LIBRA-phase1
- Combined Annual Modulation Dark Matter Search with COSINE-100 and ANAIS-112
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
- First Constraints on WIMP-Nucleon Effective Field Theory Couplings in an Extended Energy Region From LUX-ZEPLIN
- Enhancing Direct Detection of Higgsino Dark Matter
- Strong Constraints on Higgsino Dark Matter from Solar Capture
- Solar Neutrino Constraints on Inelastic Dark Matter Scattering in Light of Recent LUX-ZEPLIN Observations
- Confronting the Higgsino Interpretation of the LZ Event with the High-Energy Sideband
- Direct Detection of Electroweak-Interacting Dark Matter
- Last Electroweak WIMP Standing: Pseudo-Dirac Higgsino Status and Compact Stars as Future Probes
- The Race to Find Split Higgsino Dark Matter
- Chasing higgsino dark matter at colliders in the neutrino fog era
- The discreet charm of higgsino dark matter - a pocket review
- Higgsino Dark Matter in High-Scale Supersymmetry
- Supersymmetric Unification Without Low Energy Supersymmetry And Signatures for Fine-Tuning at the LHC
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