A detailed view at magnetic dipole strengths: The case of semi-magic 50Ti
Abstract
Magnetic dipole, M1, strengths were studied in semi-magic 50Ti up to the neutron-separation threshold by combining data from (d,p) one-neutron transfer, (γ,γ') real-photon scattering, (e,e') inelastic scattering at extreme backward angles, and (p,p') at Ep = 210 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 (1f7/2)−1(1f5/2)+1 spin-flip transitions, which were probed with the (d,p) reaction, to the overall strength in 50Ti questions the standard picture for the microscopic origin of spin-flip strength in the fp shell. For 50Ti, this letter shows that Jπ = 1+ states with larger neutron (1f7/2)−1(1f5/2)+1 spectroscopic factors do not correspond to the ones with the largest B(M1;0+1 → 1+i) strengths.
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BibTeX
@misc{kelly2026detailed,
title = {{A detailed view at magnetic dipole strengths: The case of semi-magic $^50$Ti}},
author = {B. Kelly and M. Spieker and U. Friman-Gayer and L. T. Baby and T. Beck and A. L. Conley and S. W. Finch and J. Isaak and Krishichayan and E. Litvinova and H. Pai and N. Pietralla and D. Savran and W. Tornow and N. Tsoneva and A. Volya and V. Werner},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.10843},
eprint = {2609.10843},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.10843},
}
RIS
TY - UNPB
TI - A detailed view at magnetic dipole strengths: The case of semi-magic ^50Ti
AU - B. Kelly
AU - M. Spieker
AU - U. Friman-Gayer
AU - L. T. Baby
AU - T. Beck
AU - A. L. Conley
AU - S. W. Finch
AU - J. Isaak
AU - Krishichayan
AU - E. Litvinova
AU - H. Pai
AU - N. Pietralla
AU - D. Savran
AU - W. Tornow
AU - N. Tsoneva
AU - A. Volya
AU - V. Werner
PY - 2026
DA - 2026/09/09
PB - arXiv
DO - 10.48550/arxiv.2609.10843
UR - https://arxiv.org/abs/2609.10843
AB - Magnetic dipole, M1, strengths were studied in semi-magic ^50Ti up to the neutron-separation threshold by combining data from (d,p) one-neutron transfer, (γ,γ') real-photon scattering, (e,e') inelastic scattering at extreme backward angles, and (p,p') at E_p = 210 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 ^50Ti questions the standard picture for the microscopic origin of spin-flip strength in the fp shell. For ^50Ti, this letter shows that J^π = 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 → 1^+_i) strengths.
ER -