Electroweak inelastic DM · Discriminant
From LUX-ZEPLIN to Colliders: Probing Higgsino Dark Matter
- Published
- September 8, 2026
- Identifier
- arXiv:2609.08712
Why it is here
Translates the LZ-motivated Higgsino spectrum into a short-track collider signature.
Machine-assisted summary
The authors trace the 1.1 TeV Higgsino interpretation to a nearly degenerate chargino with a sub-centimeter track, finding current LHC searches insensitive but identifying tracklet reach at future hadron and muon colliders.
Citation lineage on this map
Cites 21
- Inelastic Dark Matter Signature at High Recoil Energy in LUX-ZEPLIN and CRESSTLiangliang Su, Jin Min Yang, Wen-Na Yang · 2026
- Higgsino Above the Sea of FogJiJi Fan, Matthew Reece · 2026
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil EventKatherine Freese, Dionysios P. Theodosopoulos · 2026
- TeV Higgsino Dark Matter from LZ Nuclear Recoil to Fermi-LAT Gamma RaysLei Wu, Yang Zhang, Bin Zhu · 2026
- Fermionic Dark Matter Absorption and the High-Energy Event in LUX-ZEPLINYuanchao Lou, Chih-Ting Lu · 2026
- A PQ-Symmetric High-Scale SUSY Interpretation of the LZ High-Energy RecoilWen Yin · 2026
- Dark Matter as the Z₂ Partner of the Standard Model Higgs BosonYasunori Nomura · 2026
- Dark Matter at the Kinematic Edge: Interpreting the 248 keV LZ Nuclear-Recoil CandidateMattia Di Mauro · 2026
- A Peccei-Quinn Origin for Inelastic Electroweak Dark Matter after LUX-ZEPLINLuca Visinelli · 2026
- Search for dark matter particle interactions in an extended nuclear recoil energy window with the LUX-ZEPLIN (LZ) experimentLZ Collaboration · 2026
- Inelastic Dark Photon Dark Matter for the LUX-ZEPLIN High-Recoil Event and the Galactic Halo Gamma-Ray ExcessKimiko Yamashita · 2026
- Sub-TeV Singlino Dark Matter in light from Sagittarius A* and LUX-ZEPLIN Nuclear-Recoil EventUtpal Chattopadhyay, Debottam Das, Rahul Puri, Joydeep Roy · 2026
- Inelastic Signatures of Electroweak Dark MatterJuri Smirnov, Spencer Griffith, John F. Beacom · 2026
- TeV Higgsino Interpretation of the LZ High-Recoil Event with Intermediate-Scale Electroweak GauginosXiaokang Du, Fei Wang · 2026
- Confronting the Higgsino Interpretation of the LZ Event with the High-Energy SidebandNicholas L. Rodd, Benjamin R. Safdi, Tracy R. Slatyer, Weishuang Linda Xu · 2026
- Seasonal dark matter from the LUX-ZEPLIN high-energy eventChristopher McCabe · 2026
- Atmospheric neutrino up-scattering explanation of LZ 2026 excessSk Jeesun, Anirban Majumdar · 2026
- Axion Portal Dark Matter and the LUX-ZEPLIN High-Recoil EventJames Unwin · 2026
- Exothermic and Endothermic Inelastic Dark Matter Interpretations at LZ: Sideband Constraints and Future ProspectsJames B. Dent, Jayden L. Newstead · 2026
- Exothermic Dark Matter at LZCarlos Henrique de Lima · 2026
- Inelastic from the Other Side: Xenon Excitation Signals in Light of the LZ High-Recoil EventGuanhua Gu, Lingfeng Li, Shao-Song Tang, Yongheng Xu · 2026
Cited by 39
- Sub-TeV Singlino Dark Matter in light from Sagittarius A* and LUX-ZEPLIN Nuclear-Recoil EventUtpal Chattopadhyay, Debottam Das, Rahul Puri, Joydeep Roy · 2026
- Exothermic dark matter and the 248 keV nuclear recoil in LUX-ZEPLINHoward Baer, Vernon Barger · 2026
- Higgsino Dark Matter Interpretation of the LZ High-Recoil Event in the GNMSSM with TeV-Scale GauginosSubhadip Bisal, Junjie Cao, Fei Li · 2026
- Endothermic dark matter with a light dark photon and the LUX-ZEPLIN high-energy nuclear-recoil candidatePengxuan Zhu, Giovani Dalla Valle Garcia, Xuan-Gong Wang, Anthony W. Thomas, Martin J. White · 2026
- Transition magnetic-dipole dark matter and the LZ230616 high-recoil candidateYuxuan He · 2026
- Inelastic Dark Matter and High-Energy Recoil Signatures in LZZi-Tong Fan, Hong-Jian He, Yu-Chen Wang, Yue Zhao · 2026
- Generalized Chiral $U(1)_{B-L}$ with Inelastic Scalar Dark Matter for the LZ 248 keV EventRanjeet Kumar, Hemant Kumar Prajapati · 2026
- Nuclear Recoils from Invisible Neutron-Pair Annihilation and the LZ eventJunseok Lee, Fuminobu Takahashi, Yu-Dai Tsai · 2026
- Can a minimal radiative seesaw explain the LZ 248 keV event?Hiroshi Okada, Yoshihiro Shigekami, Jia-Jun Wu · 2026
- Boosted or Inelastic? Discriminating Interpretations of the LZ 248 keV EventSatyabrata Mahapatra, Partha Kumar Paul · 2026
- Inelastic Dark Matter at LZ from Radiative Dirac Neutrino Mass ParadigmPankaj Borah, Satyabrata Mahapatra, Newton Nath, Partha Kumar Paul · 2026
- Confronting the Higgsino Interpretation of the LZ Event with Astrophysical Uncertainties and the Solar Capture ConstraintsAditya Ghosh, Ilumi Chavez, Chris Kelso · 2026
- Effect of inelastic scalar dark matter in hidden $U(1)$ scenario after the LZ nuclear recoilArindam Das, Takaaki Nomura · 2026
- Xenon Isotope Filtering at the Kinematic Edge of Inelastic Dark MatterWaqas Ahmed, Ammara Ahmad, Mansoor Ur Rehman · 2026
- DM induced neutron disappearance as the origin of the LZ nuclear recoil eventP. Uttayarat, J. Julio, R. Primulando · 2026
- Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ EventHaipeng An, Fei Gao, Jia Liu, Minghao Liu, Changlong Xu · 2026
- Asymmetric Inelastic Dark Matter and the LUX-ZEPLIN eventNatsumi Nagata, Tsutomu T. Yanagida · 2026
- Endothermic Z'-Portal Dark Matter: LZ-LHC ComplementarityNobuchika Okada, Digesh Raut · 2026
- LUX-ZEPLIN's Stairway to Hea$\nu$en: limits on elastic scatters of dark matter from solar captureDebajit Bose, Thong T. Q. Nguyen, Akash Kumar Saha, Nirmal Raj, Tarak Nath Maity, Ranjan Laha · 2026
- The 248 keV LZ Recoil: A Possible Hint of Non-SM-Like Quark Yukawa Couplings with a Scalar-Portal Dark MatterBibhabasu De · 2026
- LZ-Motivated Pseudo-Dirac Higgsinos in the Supersymmetric 331 Model from the Supersymmetric \texorpdfstring{$SU(6)$}{SU(6)} GUT ModelImtiaz Khan, Ali Muhammad, G. Mustafa, Farruh Atamurotov, Ahmadjon Abdujabbarov, Mussawir Khan · 2026
- A closer look at the LZ 248 keV event through the lens of cosmic-ray boosted dark matterBhavesh Chauhan, Soham Sahasrabuddhe, Manibrata Sen · 2026
- Elastic toroidal vector dark matter through a dark photon in the LUX-ZEPLIN high recoil windowImtiaz Khan, Salvatore Capozziello, G. Mustafa, Farkhod Botirov, Ahmadjon Abdujabbarov, Farruh Atamurotov, Phongpichit Channuie · 2026
- Dark Diffraction at LZ from a Screened Neutral Composite BaryonHyunjoo Jung, Seong Chan Park · 2026
- Model-Independent Sideband Constraints on Inelastic Dark Matter at the LZ High-Recoil CandidateDavid Delepine, Shaaban Khalil · 2026
- The LHC is not enough: the LZ High-Recoil Event at FCC-hh and a Muon ColliderBenedikt Maier, Michael Spannowsky · 2026
- Environment-dependent mass splitting to suppress solar capture in the inelastic-doublet interpretation of the LZ eventSudhakantha Girmohanta, Tae Hyun Jung · 2026
- Sneaky Sneutrino Scattering at LZKevin Langhoff, Huangyu Xiao · 2026
- Heavy Higgsino Dark Matter With Low Reheating in View of the LZ High-Recoil EventC. Pallis · 2026
- The LZ event with a two-state dark matter haloVinicius Oliveira · 2026
- GAIA meets LZ: a high velocity tail-tale sign for dark matterAnirban Das, Subhabrata Majumdar, Manibrata Sen, Amogh Srivastav · 2026
- Endothermic Dark Matter at LZ from a Decaying ParentYongsoo Jho, Sanghwan Kim, Seong Chan Park · 2026
- Decaying Dark Matter for the Exothermic Recoil at LZYongsoo Jho, Sanghwan Kim, Seong Chan Park · 2026
- Constraints on Complex Electroweak WIMPs from Solar CaptureJuan P. Luengas, Maxim Pospelov, Harikrishnan Ramani · 2026
- Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark MatterSubhojit Roy, Pedro Schwaller, Carlos E. M. Wagner · 2026
- From the LZ Event to Grand Unification: Heavy Higgsinos and Proton DecayShihwen Hor, Natsumi Nagata, Tsutomu T. Yanagida · 2026
- Environment-Dependent Annihilation of Axion-Coupled Higgsino Dark MatterKwang Sik Jeong, Fuminobu Takahashi · 2026
- One Event, Two Frontiers: From LZ to LHCMd Sadique Anwar, Nivedita Ghosh, Sahabub Jahedi, Tarak Nath Maity · 2026
- Can Nuclear Recoils and Solar Neutrinos Resolve the Composition of Singlino-Higgsino Dark Matter?Jingwei Lian, Jin Min Yang · 2026
Metadata comes from arXiv. Summaries and placement are machine-assisted; inclusion is not endorsement or peer review.