An Axial-Vector Leptophilic Fifth Force Sourced by Solar Neutrinos
Rundong Fang, Ji-Heng Guo, Jia Liu, Xiao-Ping Wang, YanLi Zhao
TL;DR
The paper introduces a purely leptophilic axial-vector fifth force mediated by a light $A'$ that couples axially to charged leptons and left-handed neutrinos, with solar neutrinos acting as an extended Sun–Earth source. It analyzes two anomaly-free realizations ($L^{AV}_\mu$ and $L^{AV}_\mu-L^{AV}_\tau$) and derives the $A'$ field sourced at Earth, leading to a diurnal, sign-changing contribution to the muon anomalous magnetic moment $(g-2)_\mu$ in storage rings, plus a time-independent offset. Using muon $g-2$ data, it derives bounds $g' \lesssim \mathcal{O}(10^{-19})$ for a light mediator, while electron-channel constraints yield $g'_e \lesssim \mathcal{O}(10^{-22})$ via spin-sensor mappings; accounting for day–night modulation strengthens these muon bounds by about an order of magnitude. The work highlights the potential for time-domain particle-physics probes leveraging solar neutrino fluxes to constrain new long-range forces and underscores model independence via anomaly-free charge patterns. Overall, the solar-neutrino–sourced axial-vector interaction provides a novel avenue to test leptophilic new physics with current and near-future precision experiments.
Abstract
We investigate long-range, purely leptophilic axial-vector interactions mediated by a light gauge boson $A'$ that couples to charged leptons and, by weak symmetry, to left-handed neutrinos. We analyze two realizations, a minimal effective model with muon-only couplings and an anomaly-free axial $U(1)'$ with inter-generation cancellations. In both cases, the solar neutrino flux acts as an extended current that sources a macroscopic $A'$ field at Earth, with spatial components aligned along the Sun-Earth direction. This field produces a distinctive signature in storage-ring measurements of the muon anomalous magnetic moment, $(g-2)_μ$, namely a diurnal, sign-changing contribution that is positive during daytime and negative at night, superimposed on a time-independent positive offset. We obtain bounds $g' \lesssim {O}(10^{-19})$ in both model frameworks for a light, effectively massless mediator. For completeness, we map the solar-neutrino-sourced potential to electron spin-sensor experiments and find $g' \lesssim {O}(10^{-22})$ in the electron channel.
