Dark Transition Magnetic Moments of Majorana Neutrinos Mediated by a Dark Photon

TL;DR

This paper proposes a dark sector model to generate observable Majorana neutrino transition magnetic moments via scalar loops, overcoming Standard Model suppressions, and analyzes its experimental constraints and phenomenological implications.

Contribution

It introduces a novel dark sector mechanism for Majorana neutrino magnetic moments that avoids fermion loop cancellations and explores its experimental viability.

Findings

Scalar loops generate a chirally enhanced dark TMM.

Experimental constraints from cLFV and collider searches are highly restrictive.

High-energy probes dominate over direct solar neutrino limits.

Abstract

Standard Model predictions for Majorana neutrino transition magnetic moments (TMMs) are subject to severe chiral and GIM-like suppressions, rendering them vanishingly small. To dynamically generate a macroscopic TMM, we propose a dark sector framework featuring a $U(1)_D$ gauge symmetry, a vector-like lepton doublet, and two complex dark scalars. We demonstrate that while fermion-radiated loop amplitudes identically cancel due to Majorana self-conjugacy, a chirally enhanced dark TMM is successfully generated exclusively through scalar-radiated loops. This mechanism safely shifts the required chirality flip onto the heavy internal fermion line and utilizes a misaligned double-scalar mixing in flavor space to evade the Majorana antisymmetry prohibition. We systematically confront this tensor portal framework with multi-frontier experimental constraints. Since the dark TMM generation is inextricably linked to charged lepton flavor violation, the internal Yukawa couplings are stringently capped by the latest $\mu \to e \gamma$ limits from MEG II. Concurrently, the visible-dark kinetic mixing portal is heavily bottlenecked by missing energy and mono-photon searches at NA64 and BaBar. Our global phenomenological analysis reveals that the synergistic theoretical upper bound dictated by these indirect high-energy probes completely eclipses the direct scattering constraints from Borexino. This establishes a strict phenomenological hierarchy: high-intensity cLFV probes and accelerator-based dark sector searches jointly possess the overwhelmingly dominant exclusionary power over direct solar neutrino limits for such microscopic magnetic moment models.