Magnetic dipole, $M1$, strengths were studied in semimagic ${}^{50}\mathrm{Ti}$ up to the neutron-separation threshold by combining data from $(d,p)$ one-neutron transfer, $(\gamma ,{\gamma }^{\prime })$ real-photon scattering, $(e,e^{\prime })$ inelastic scattering at extreme backward angles, and $(p,p^{\prime })$ at $E_p=210\mathrm{MeV}$ and extreme forward angles. The combination of all probes provided unique access to the neutron spin-flip contribution and the possibility to evaluate its role in generating the spin-flip $M1$ strengths. The small contribution of the neutron $(1f_{7/2}{)}^{-1}(1f_{5/2}{)}^{+1}$ spin-flip transitions, which were probed with the $(d,p)$ reaction, to the overall strength in ${}^{50}\mathrm{Ti}$ questions the standard picture for the microscopic origin of spin-flip strength in the $fp$ shell. For ${}^{50}\mathrm{Ti}$, this Letter shows that $J^{\pi }=1^{+}$ states with larger neutron $(1f_{7/2}{)}^{-1}(1f_{5/2}{)}^{+1}$ spectroscopic factors do not correspond to the ones with the largest $B(M1;0_1^{+}\to 1_i^{+})$ strengths.

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• Collective levels
• Direct reactions
• Gamma-ray strength functions
• Giant resonances
• Nuclear reactions
• Nuclear structure & decays
• Nuclear transition rates
• Photonuclear reactions
• Spectroscopic factors & electromagnetic moments
• Transfer reactions