The LRIS model explains the B→Kμμ anomaly with ΔC9 ≈ -1 and ΔC10 ≈ 0 through a non-decoupling box diagram while suppressing Bs mixing via GIM-like phases and satisfying constraints.
Pilaftsis, Radiatively induced neutrino masses and large Higgs–neutrino couplings in the Standard Model with Ma- jorana fields, Z
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Explaining the $B \to K\mu^+\mu^-$ Anomaly in the Left-Right Inverse Seesaw Model
The LRIS model explains the B→Kμμ anomaly with ΔC9 ≈ -1 and ΔC10 ≈ 0 through a non-decoupling box diagram while suppressing Bs mixing via GIM-like phases and satisfying constraints.