The LZ event with a two-state dark matter halo
hep-ph, astro-ph.HE
Submitted: 2026-09-28
Updated: 2026-09-28
Comments: 11 pages, 7 figures
Code: https://github.com/veragluscevic/dmdd
License: http://creativecommons.org/licenses/by/4.0/
The gist: The LUX-ZEPLIN (LZ) experiment has reported a single nuclear-recoil candidate at E R 248 keV.
Terminology
Abstract
The LUX-ZEPLIN (LZ) experiment has reported a single nuclear-recoil candidate at E R 248 keV. LZ interprets it in terms of inelastic dark matter that scatters endothermically from its ground state, χ 1 N to χ 2 N. In pseudo-Dirac models the excited state χ 2 can survive to the present day, and exothermic scattering, χ 2 N to χ 1 N, is then also open. The published LZ intervals do not describe this case. We rebuild the LZ statistical inference and validate it against the published intervals. We then apply it to a halo that contains a fraction f of χ 2. For f 10-5 -- 10-2, depending on the mass splitting, the exothermic contribution dominates. For f=1/2 the cross section required by the candidate drops by factors of 80 to 1.6 times10 4 for δ= 250 -- 350 keV, and the kinematic cutoff of the endothermic signal disappears. A benchmark that explains the event with χ 1 alone lies a factor of 30 above the upper limit when half of the halo is χ 2.
Sources
- Planck 2018 results. VI. Cosmological parameters
- Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
- The Effective Field Theory of Dark Matter Direct Detection
- Model-independent WIMP Scattering Responses and Event Rates: A Mathematica Package for Experimental Analysis
- Dark Matter at the Kinematic Edge: Interpreting the 248 keV LZ Nuclear-Recoil Candidate
- Inelastic Singlet-Doublet Fermion Dark Matter in light of the 248 keV LZ event
- Exothermic Dark Matter
- Inelastic Dark Matter at LZ from Radiative Dirac Neutrino Mass Paradigm
- Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ Event
- Hadrophilic inelastic freeze-in dark matter in q 1-q 2 gauge extension and the high energy LZ event
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