Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
- 1Weinberg Institute for Theoretical Physics , Department of Physics , The University of Texas at Austin , Austin , TX 78712 , USA
Abstract
We propose Higgsino dark matter as a potential interpretation of the 248 keV nuclear-recoil event of interest reported by the LUX-ZEPLIN (LZ) experiment. LZ studied several rare background processes and detector effects in detail, but did not identify any as a likely explanation of the event. A nearly pure Higgsino naturally realizes inelastic dark matter through the off-diagonal Z coupling of two nearly degenerate neutral Majorana states separated by a mass splitting δ. The same electroweak interaction fixes the inelastic Higgsino-nucleon scattering cross section, rather than leaving it as a free parameter. We show that the predicted Higgsino inelastic scattering cross section approaches the published LZ two-sided 90% confidence interval for a Higgsino mass mH̃∼1 TeV and a mass splitting δ∼350 keV.
Related
- Higgsino dark matter compatible with the LUX-ZEPLIN high-energy nuclear-recoil event and IceCube constraints
- Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark Matter
- A Vector-Like Lepton Interpretation of the High-Energy Nuclear Recoil Candidate in LUX-ZEPLIN
- Sub-TeV Singlino Dark Matter in light from Sagittarius A∗ and LUX-ZEPLIN Nuclear-Recoil Event
- Higgsino dark matter in the Starobinsky supergravity with the MSSM in light of the LUX-ZEPLIN event
BibTeX
@misc{freese2026higgsino,
title = {{Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event}},
author = {Katherine Freese and Dionysios P. Theodosopoulos},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.01583},
eprint = {2609.01583},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.01583},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
AU - Katherine Freese
AU - Dionysios P. Theodosopoulos
PY - 2026
DA - 2026/09/01
PB - arXiv
DO - 10.48550/arxiv.2609.01583
UR - https://arxiv.org/abs/2609.01583
AB - We propose Higgsino dark matter as a potential interpretation of the 248 keV nuclear-recoil event of interest reported by the LUX-ZEPLIN (LZ) experiment. LZ studied several rare background processes and detector effects in detail, but did not identify any as a likely explanation of the event. A nearly pure Higgsino naturally realizes inelastic dark matter through the off-diagonal Z coupling of two nearly degenerate neutral Majorana states separated by a mass splitting δ. The same electroweak interaction fixes the inelastic Higgsino-nucleon scattering cross section, rather than leaving it as a free parameter. We show that the predicted Higgsino inelastic scattering cross section approaches the published LZ two-sided 90% confidence interval for a Higgsino mass m_H̃∼1 TeV and a mass splitting δ∼350 keV.
SN - 2331-8422
ER -