Boosted or Inelastic? Discriminating Interpretations of the LZ 248 keV Event
hep-ph, astro-ph.CO, hep-ex, hep-th
Submitted: 2026-09-13
Updated: 2026-09-13
Comments: 8+2 pages, 3 captioned figures, 0 tables
License: http://creativecommons.org/licenses/by/4.0/
The gist: The LUX-ZEPLIN experiment has reported a single nuclear recoil candidate at E R = 248 plus or minus 23(stat) plus or minus 23(sys) keV, disfavouring the background-only hypothesis at a global
Terminology
Abstract
The LUX-ZEPLIN experiment has reported a single nuclear recoil candidate at E R = 248 plus or minus 23(stat) plus or minus 23(sys) keV, disfavouring the background-only hypothesis at a global significance of 2.6σ. The difficulty such an event poses is not the recoil energy itself but the absence of any accompanying excess at low energy as elastic scattering of halo dark matter yields a monotonically falling spectrum, and supplying the required momentum transfer q 246 MeV already demands m χ 79 GeV. We confront the event with the two kinematically distinct mechanisms that evade this limitation, endothermic inelastic dark matter, in which a mass splitting δ about O(100) keV forbids low-energy recoils and boosted dark matter, in which a light relativistic flux supplies the momentum, treating both with the same model-independent scalar--scalar, pseudoscalar--scalar and pseudoscalar--pseudoscalar effective operators. The two scenarios prove spectrally distinguishable. The inelastic spectra sit near the observed energy for every operator, placing only 6 -- 17% of events below 150 keV, whereas the boosted spectra depend critically on the operator: the scalar and pseudoscalar--scalar interactions place 99% and 92% of their events below 150 keV, while the pseudoscalar--pseudoscalar interaction places 75% above it. Momentum dependence is thus essential to the boosted interpretation, but in the inelastic case it trades against the splitting, the preferred δ decreasing monotonically from O ss to O ps to O pp. Because the scenarios differ across the whole high-energy window, a handful of additional events would separate them, placing the question within reach of the full LZ exposure.
Sources
- A direct empirical proof of the existence of dark matter
- Planck 2018 results. VI. Cosmological parameters
- The Waning of the WIMP? A Review of Models, Searches, and Constraints
- Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
- WIMP Dark Matter Search using a 3.1 Tonne-Year Exposure of the XENONnT Experiment
- Dark Matter Search Results from 1.54 Tonne$\cdot$Year Exposure of PandaX-4T
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
- Dark Matter at the Kinematic Edge: Interpreting the 248 keV LZ Nuclear-Recoil Candidate
- Inelastic Dark Photon Dark Matter for the LUX-ZEPLIN High-Recoil Event and the Galactic Halo Gamma-Ray Excess
- Confronting the Higgsino Interpretation of the LZ Event with the High-Energy Sideband
- Inelastic Self-interacting Dark Matter and LUX-ZEPLIN 248 keV Event in a Dirac Modular Inverse Seesaw
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