Abstract
The Fermilab Muon g − 2 collaboration recently announced the first result of measurement of the muon anomalous magnetic moment (g − 2), which confirmed the previous result at the Brookhaven National Laboratory and thus the discrepancy with its Standard Model prediction. We revisit low-scale supersymmetric models that are naturally capable to solve the muon g − 2 anomaly, focusing on two distinct scenarios: chargino-contribution dominated and pure-bino-contribution dominated scenarios. It is shown that the slepton pair-production searches have excluded broad parameter spaces for both two scenarios, but they are not closed yet. For the chargino-dominated scenario, the models with \( {m}_{{\tilde{\mu}}_{\mathrm{L}}}\gtrsim {m}_{{\tilde{\chi}}_1^{\pm }} \) are still widely allowed. For the bino-dominated scenario, we find that, although slightly non-trivial, the region with low tan β with heavy higgsinos is preferred. In the case of universal slepton masses, the low mass regions with \( {m}_{\tilde{\mu}} \) ≲ 230 GeV can explain the g − 2 anomaly while satisfying the LHC constraints. Furthermore, we checked that the stau-bino coannihilation works properly to realize the bino thermal relic dark matter. We also investigate heavy staus case for the bino-dominated scenario, where the parameter region that can explain the muon g − 2 anomaly is stretched to \( {m}_{\tilde{\mu}} \) ≲ 1.3 TeV.
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Endo, M., Hamaguchi, K., Iwamoto, S. et al. Supersymmetric interpretation of the muon g – 2 anomaly. J. High Energ. Phys. 2021, 75 (2021). https://doi.org/10.1007/JHEP07(2021)075
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DOI: https://doi.org/10.1007/JHEP07(2021)075