PreprintCC BY 4.0arXiv
Inelastic B−L scalar dark matter and the LUX-ZEPLIN event
- 1Department of Physics and Astronomy , University of Alabama , Tuscaloosa , Alabama 35487 , USA
- 2Department of Physics , Hokkaido University , Sapporo 060-0810 , Japan
Abstract
We show that our previously proposed inelastic scalar dark matter (DM) model in gauged U(1)B−L symmetry naturally accounts for the 2.6σ high-energy recoil event recently reported by the LUX-ZEPLIN (LZ) collaboration. To satisfy the thermal relic abundance, TeV-scale scalar DM S with mS ≃ mZ'/2 for resonant annihilation and the gauge coupling constant gB−L ∼ 0.5 are required, where mZ′ is the mass of U(1)B−L gauge boson Z′. The resulting predicted DM-nucleon inelastic cross section of σSI ∼ 10−45 cm2 is in excellent agreement with the LZ event. This scenario can be decisively tested for future collider searches for Z′ boson resonance.
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BibTeX
@misc{okada2026inelastic,
title = {{Inelastic $B-L$ scalar dark matter and the LUX-ZEPLIN event}},
author = {Nobuchika Okada and Osamu Seto},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.06909},
eprint = {2609.06909},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.06909},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Inelastic B−L scalar dark matter and the LUX-ZEPLIN event
AU - Nobuchika Okada
AU - Osamu Seto
PY - 2026
DA - 2026/09/07
PB - arXiv
DO - 10.48550/arxiv.2609.06909
UR - https://arxiv.org/abs/2609.06909
AB - We show that our previously proposed inelastic scalar dark matter (DM) model in gauged U(1)_B−L symmetry naturally accounts for the 2.6σ high-energy recoil event recently reported by the LUX-ZEPLIN (LZ) collaboration. To satisfy the thermal relic abundance, TeV-scale scalar DM S with m_S ≃ m_Z'/2 for resonant annihilation and the gauge coupling constant g_B−L ∼ 0.5 are required, where m_Z^′ is the mass of U(1)_B−L gauge boson Z^′. The resulting predicted DM-nucleon inelastic cross section of σ_SI ∼ 10^−45 cm^2 is in excellent agreement with the LZ event. This scenario can be decisively tested for future collider searches for Z^′ boson resonance.
SN - 2331-8422
ER -