Electroweak inelastic DM · Interpretation
Heavy Higgsino Interpretation of the LZ Event
- Published
- September 8, 2026
- Identifier
- arXiv:2609.09385
Why it is here
Sideband and IceCube constraints push a pure-Higgsino explanation toward a nonthermally produced ultraheavy state.
Machine-assisted summary
The author jointly fits the LZ recoil and empty high-energy sideband for pure Higgsino dark matter, then incorporates solar-capture limits and identifies an ultraheavy nonthermal region as the surviving interpretation.
Citation lineage on this map
Cites 9
- 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
- A PQ-Symmetric High-Scale SUSY Interpretation of the LZ High-Energy RecoilWen Yin · 2026
- Dark Matter at the Kinematic Edge: Interpreting the 248 keV LZ Nuclear-Recoil CandidateMattia Di Mauro · 2026
- Strong Constraints on Higgsino Dark Matter from Solar CaptureMaxim Pospelov, Harikrishnan Ramani · 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
- 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
Cited by 53
- Solar Capture Tests of Inelastic Dark Matter after the LZ High-Recoil EventMattia Di Mauro, Halim Shaikh · 2026
- Higgsino Dark Matter Interpretation of the LZ High-Recoil Event in the GNMSSM with TeV-Scale GauginosSubhadip Bisal, Junjie Cao, Fei Li · 2026
- A Vector-Like Lepton Interpretation of the High-Energy Nuclear Recoil Candidate in LUX-ZEPLINFatemeh Elahi, Pedro Schwaller · 2026
- Mixing-suppressed inelastic dark matter: a minimal model for the LZ 248 keV eventSeung J. Lee, Taewook Youn · 2026
- Inelastic Dark Matter and High-Energy Recoil Signatures in LZZi-Tong Fan, Hong-Jian He, Yu-Chen Wang, Yue Zhao · 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
- Hadrophilic inelastic freeze-in dark matter in $q_1-q_2$ gauge extension and the high energy LZ eventXiao-Gang He, Xuan Hong, Sk Jeesun · 2026
- DM induced neutron disappearance as the origin of the LZ nuclear recoil eventP. Uttayarat, J. Julio, R. Primulando · 2026
- Inferring dark matter masses and interactions from high recoil energy events in LUX-ZEPLINStefano Palmisano, Michele Tammaro, Andrea Tesi · 2026
- A possible interpretation of the LUX-ZEPLIN recoil event in the 2HD+a scenarioGiorgio Arcadi, Mattia di Mauro, Abdelhak Djouadi, Farinaldo Queiroz · 2026
- Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ EventHaipeng An, Fei Gao, Jia Liu, Minghao Liu, Changlong Xu · 2026
- Galactic Endothermic Production and Exothermic Detection of Excited Dark Matter: Implications for LUX-ZEPLINChuan-Yang Xing · 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
- The high-velocity dark matter halo of the Milky Way in light of the LZ 248 keV eventCiaran A. J. O'Hare · 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
- Resurrecting Electroweak Dark Matter via Type-II Seesaw in light of recent LZ EventPartha Kumar Paul, Sujit Kumar Sahoo, Narendra Sahu, Shashwat Sharma · 2026
- Kaluza--Klein Dark-Photon Mediation of Inelastic Dark Matter at LUX-ZEPLINWaqas Ahmed, George K. Leontaris · 2026
- The 248 keV LZ Recoil: A Possible Hint of Non-SM-Like Quark Yukawa Couplings with a Scalar-Portal Dark MatterBibhabasu De · 2026
- The LUX-ZEPLIN Event as Hyperfine Spectroscopy of Composite Dark MatterJie Sheng, Kairui Zhang · 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
- Dark Diffraction at LZ from a Screened Neutral Composite BaryonHyunjoo Jung, Seong Chan Park · 2026
- A Simple Dark Matter Model to Explain the LZ Event and Galactic Center ExcessCaleb Gemmell, Dan Hooper, Gordan Krnjaic · 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
- Solar capture and annihilation of fermionic and scalar dark matter motivated by the LUX-ZEPLIN high-recoil candidateAntonio Capolupo, Gabriele Pisacane, Raoul Serao · 2026
- Inelastic dark matter mediated by natural dark photonJie Tang, Pei-Hong Gu · 2026
- Sneaky Sneutrino Scattering at LZKevin Langhoff, Huangyu Xiao · 2026
- Heavy Higgsino Dark Matter at the Scale of the Vanishing Higgs QuarticJames Unwin · 2026
- Heavy Inert Doublet Reconciles LZ and IceCubeHitoshi Murayama, Bea Noether · 2026
- A Narrow Neutrino Window for the LZ EventVedran Brdar, Dibya S. Chattopadhyay · 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
- Does the High Energy LUX-ZEPLIN Event Suggest Hyperfine Atomic Dark Matter?Prolay Chanda, Bhaskar Das, Sagnik Mukherjee · 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
- Thermal Higgsino Dark Matter in GmSUGRA for the LZ Event and Solar-Neutrino ConstraintImtiaz Khan, Waqas Ahmed, Tianjun Li, Shabbar Raza, Ali Muhammad · 2026
- Inelastic Dark Matter from a Higher-Dimensional Operator: The LUX-ZEPLIN High-Recoil Event and Thermal RelicDebajyoti Choudhury, Jaydeb Das, Divya Sachdeva · 2026
- From the LZ Event to Grand Unification: Heavy Higgsinos and Proton DecayShihwen Hor, Natsumi Nagata, Tsutomu T. Yanagida · 2026
- Higgsino dark matter compatible with the LUX-ZEPLIN high-energy nuclear-recoil event and IceCube constraintsKatherine Freese, Dionysios P. Theodosopoulos · 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
- Testing Dark Matter Coscattering with the High-Energy LZ RecoilSreemanti Chakraborti, Soumyajit Datta · 2026
- Can Nuclear Recoils and Solar Neutrinos Resolve the Composition of Singlino-Higgsino Dark Matter?Jingwei Lian, Jin Min Yang · 2026
- A scalar-extended ${\rm U(1)_{L_{\mu}-L_{\tau}}}$ explanation of the LUX-ZEPLIN 248 keV excessDipankar Pradhan, Abhik Sarkar · 2026
Metadata comes from arXiv. Summaries and placement are machine-assisted; inclusion is not endorsement or peer review.