Solar Neutrino Probes of Light New Physics: Updated Limits from LUX-ZEPLIN Experiment

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Main Authors: Demirci, Mehmet, Mustamin, M. Fauzi
Format: Preprint
Published: 2026
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author Demirci, Mehmet
Mustamin, M. Fauzi
author_facet Demirci, Mehmet
Mustamin, M. Fauzi
contents The recent low-energy electron recoil (ER) results reported by the LUX-ZEPLIN (LZ) experiment have established the most stringent constraints to date on new physics scenarios, specifically for solar axion-like particles with keV-scale masses and mirror dark matter. Motivated by this enhanced sensitivity and the resulting restrictive limits, our present work focuses on probing light mediator models via elastic neutrino-electron scattering induced by solar neutrinos. We specifically consider two broad classes of new physics scenarios: (i) universal light mediator models consistent with Lorentz invariance, including scalar, vector, and tensor interactions, and (ii) anomaly-free leptophilic $U(1)'$ gauge extensions featuring a new vector mediator associated with the $L_e-L_μ$, $L_e-L_τ$, $L_μ-L_τ$, and $L_e+2L_μ+2L_τ$ symmetries. By incorporating contributions from these interactions into the neutrino-electron scattering cross-section and utilizing the most precise solar neutrino flux predictions, we analyze the latest LZ ER datasets. We report novel constraints on the coupling-mass parameter space for these models. Furthermore, we contextualize our findings by comparing them with established bounds from various laboratory, cosmological, and astrophysical sources. Our analysis demonstrates that LZ data provide significantly improved limits in previously unconstrained regions of the parameter space.
format Preprint
id arxiv_https___arxiv_org_abs_2603_19467
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Solar Neutrino Probes of Light New Physics: Updated Limits from LUX-ZEPLIN Experiment
Demirci, Mehmet
Mustamin, M. Fauzi
High Energy Physics - Phenomenology
The recent low-energy electron recoil (ER) results reported by the LUX-ZEPLIN (LZ) experiment have established the most stringent constraints to date on new physics scenarios, specifically for solar axion-like particles with keV-scale masses and mirror dark matter. Motivated by this enhanced sensitivity and the resulting restrictive limits, our present work focuses on probing light mediator models via elastic neutrino-electron scattering induced by solar neutrinos. We specifically consider two broad classes of new physics scenarios: (i) universal light mediator models consistent with Lorentz invariance, including scalar, vector, and tensor interactions, and (ii) anomaly-free leptophilic $U(1)'$ gauge extensions featuring a new vector mediator associated with the $L_e-L_μ$, $L_e-L_τ$, $L_μ-L_τ$, and $L_e+2L_μ+2L_τ$ symmetries. By incorporating contributions from these interactions into the neutrino-electron scattering cross-section and utilizing the most precise solar neutrino flux predictions, we analyze the latest LZ ER datasets. We report novel constraints on the coupling-mass parameter space for these models. Furthermore, we contextualize our findings by comparing them with established bounds from various laboratory, cosmological, and astrophysical sources. Our analysis demonstrates that LZ data provide significantly improved limits in previously unconstrained regions of the parameter space.
title Solar Neutrino Probes of Light New Physics: Updated Limits from LUX-ZEPLIN Experiment
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2603.19467