Loop-Level Lepton Flavor Violation and Diphoton Signals in the Minimal Left-Right Symmetric Model
Shufang Qiang, Peiwen Wu, Yongchao Zhang
TL;DR
The paper analyzes 1-loop radiative couplings of a light $H_3$ in the minimal LRSM, focusing on lepton flavor-violating (LFV) and lepton flavor-conserving (LFC) couplings to charged leptons and the $H_3\gamma\gamma$ diphoton channel, generated by heavy LRSM states such as the RHNs $N_i$, the $W_R$, and charged scalars. It derives the dependence of these couplings on the right-handed scale $v_R$ and shows that current laboratory and astrophysical data impose strong bounds, with gamma-ray observations of SN1987A providing the leading constraint $v_R \gtrsim 2\times 10^{9}$ GeV; future high-precision muon experiments and supernova observations could extend sensitivity to $v_R \sim 5\times 10^{9}$ GeV and $6\times 10^{11}$ GeV, respectively. The work also highlights rich phenomenology for a light $H_3$, including LFV decays $\ell_\beta \to \ell_\alpha + X$ and diphoton decays, and emphasizes the complementarity of laboratory and astrophysical probes in testing LRSM parameter space. Overall, it demonstrates that radiative $H_3$ couplings provide a powerful, multi-pronged test of the LRSM and the scale of $SU(2)_R$ breaking.
Abstract
The left-right symmetric model (LRSM) could not only restore parity of the weak interaction, but also provide natural explanations of the tiny active neutrino masses via the seesaw mechanisms. The $SU(2)_R$-breaking scalar $H_3$ can induce lepton flavor violating (LFV) effects in the minimal version of LRSM at the 1-loop order, originating from the mixing of heavy right-handed neutrinos. If $H_3$ is light, say below the GeV scale, it will lead to rich signals, e.g. the LFV muon and tauon decays $\ell_β\to \ell_α+ X$ ($X$ being either visible or invisible final states) and the anomalous supernova signatures. Combined with the diphoton coupling of $H_3$, the right-handed scale $v_R$ is excluded up to $2\times10^9$ GeV. In the future, the $v_R$ scale can be probed up to $5\times10^9$ GeV in high-precision muon experiments, and further up to $6\times10^{11}$ GeV by supernova observations.
