Other endothermic DM · Interpretation
Did LZ see modified gravity?
- Published
- September 14, 2026
- Identifier
- arXiv:2609.15118
Why it is here
Uses the recoil as a probe of the expansion history before nucleosynthesis rather than only of particle parameters.
Machine-assisted summary
The author fits endothermic freeze-in dark matter to the event during a pre-BBN era of modified cosmic expansion, using the relic abundance together with collider and cosmological bounds to select viable histories.
Citation lineage on this map
Cites 27
- 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
- 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
- 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
- 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
- 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
- Inelastic B-L scalar dark matter and the LUX-ZEPLIN eventNobuchika Okada, Osamu Seto · 2026
- LZ nuclear recoil event from inelastic singlet-doublet scalar dark matterDisha Bandyopadhyay, Debasish Borah, Pankaj Borah · 2026
- Inelastic Singlet-Doublet Fermion Dark Matter in light of the 248 keV LZ eventDebasish Borah, Sujit Kumar Sahoo, Narendra Sahu, Shashwat Sharma · 2026
- Not so good νs for Higgsino dark matter as LZ excess: stringent limits from Super-Kamiokande and IceCubeDebajit Bose, Akash Kumar Saha, Deep Jyoti Das, Rinchen Sherpa, Abhijeet Singh, Durba Ghosh, Jaya Doliya, Subhadip Bouri, Biprajit Mondal, Ranjini Mondol, Nirmal Raj, Ranjan Laha · 2026
- A Warped Extra Dimensional Candidate for the LZ 248 keV EventVincent S. H. Lee, Lisa Randall · 2026
- Can a minimal radiative seesaw explain the LZ 248 keV event?Hiroshi Okada, Yoshihiro Shigekami, Jia-Jun Wu · 2026
- A Freeze-In Interpretation of the LZ High-Energy Nuclear Recoil EventD. Cabo-Almeida, F. Costa, D. Feiteira, V. Oliveira · 2026
Cited by 18
- Sub-TeV Singlino Dark Matter in light from Sagittarius A* and LUX-ZEPLIN Nuclear-Recoil EventUtpal Chattopadhyay, Debottam Das, Rahul Puri, Joydeep Roy · 2026
- Galactic Endothermic Production and Exothermic Detection of Excited Dark Matter: Implications for LUX-ZEPLINChuan-Yang Xing · 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
- 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
- Environment-dependent mass splitting to suppress solar capture in the inelastic-doublet interpretation of the LZ eventSudhakantha Girmohanta, Tae Hyun Jung · 2026
- Inelastic dark matter mediated by natural dark photonJie Tang, Pei-Hong Gu · 2026
- Limits on Primordial Black Hole Evaporation from LUX-ZEPLINJitumani Kalita · 2026
- Heavy Higgsino Dark Matter With Low Reheating in View of the LZ High-Recoil EventC. Pallis · 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
- One Event, Two Frontiers: From LZ to LHCMd Sadique Anwar, Nivedita Ghosh, Sahabub Jahedi, Tarak Nath Maity · 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.