Rare Higgs Decay into a Photon and a Z Boson in Radiatively-Driven Natural Supersymmetry
E. A. Reyes R., C. A. Lopez A., O. R. Torrijo G., D. G. Melo P
TL;DR
The study revisits the rare Higgs decay $h\rightarrow Z\gamma$ in the SM, incorporating full LO, NLO QCD, and two-loop EW corrections across four renormalization schemes for the coupling, highlighting a ~4% variation in the width within the current Higgs mass uncertainty. It then analyzes this decay in the MSSM within Radiatively-Driven Natural SUSY (RNS), using NUHM at the GUT scale and RGEs to obtain the EW-scale spectrum and one-loop amplitudes, with dominant chargino contributions in many regions. The results show that $\Gamma_{Z\gamma}$ can reach ~7.5 keV (about 20% above the SM NLO average) for parameter choices that also yield $M_h\approx125$ GeV, but at the cost of electroweak fine-tuning $\Delta_{EW} \gtrsim 100$, signaling a tension between naturalness and observable deviations. Overall, the RNS scenario offers a mildly better description than the SM in light of recent ATLAS measurements, and future HL-LHC or FCC-ee measurements could decisively test 10–20% level deviations in this rare Higgs channel.
Abstract
In this article, we study the rare decay process in which a Higgs boson decays into a $Z$ boson and a photon. In the first part of the paper, we analyze the Standard Model (SM) contributions to the corresponding decay width, including the full leading-order result, two-loop $O(α_s)$ QCD corrections, and the recently reported two-loop $O(α)$ electroweak corrections, evaluated under four different $α$ renormalization schemes. The dependence on the Higgs boson mass is studied within the experimentally allowed range reported by the LHC. In the considered schemes, a non-negligible variation of about $4\%$ is found when the mass is varied within its current experimental uncertainty. In the second part of the paper, we analyze the leading-order contributions to the same process within the Minimal Supersymmetric Standard Model (MSSM). The spectrum of soft SUSY-breaking parameters and SUSY particle masses at the electroweak scale, which enter the computation of the one-loop amplitudes contributing to the decay width, is obtained by evolving the GUT-scale parameters of a Radiatively-Driven Natural Supersymmetry (RNS) model with non-universal Higgs boson masses. Variations of the RNS parameters can enhance the average SM prediction by up to $\sim20\%$, reaching a value of $\sim7.5~$keV, while still satisfying the Higgs boson mass constraint. However, this comes at the cost of allowing a moderately large fine-tuning parameter, with values exceeding $100$, thereby placing the model outside its most natural parameter region. The predicted decay width in the RNS scenario is closer to the recent ATLAS RUN 2 + 3 combined measurement than the SM expectation.
