Electromagnetic moments of the antimony isotopes ¹¹²¯¹³³Sb

Date

2023

Authors

Lechner, S.
Miyagi, T.
Xu, Z.Y.
Bissell, M.L.
Blaum, K.
Cheal, B.
Devlin, C.S.
Garcia Ruiz, R.F.
Ginges, J.S.M.
Heylen, H.

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Physics Letters B: Nuclear Physics and Particle Physics, 2023; 847:138278-1-138278-9

Statement of Responsibility

S. Lechner, T. Miyagi, Z.Y. Xu, M.L. Bissell, K. Blaum, B. Cheal, C.S. Devlin, R.F. Garcia Ruiz, J.S.M. Ginges, H. Heylen, J.D. Holt, P. Imgram, A. Kanellakopoulos, Á. Koszorús, S. Malbrunot-Ettenauer, R. Neugart, G. Neyens, W. Nörtershäuser, P. Plattner, L.V. Rodríguez, G. Sanamyan, S.R. Stroberg, Y. Utsuno, X.F. Yang, D.T. Yordanov

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Abstract

Nuclear moments of the antimony isotopes (113−133)Sb are measured by collinear laser spectroscopy and used to benchmark phenomenological shell-model and ab initio calculations in the valence-space in-medium similarity renormalization group (VS-IMSRG). The shell-model calculations reproduce the electromagnetic moments over all Sb isotopes when suitable effective 𝑔-factors and charges are employed. Good agreement is achieved by VSIMSRG for magnetic moments on the neutron-deficient side for both odd-even and odd-odd Sb isotopes while its results deviate from experiment on the neutron-rich side. When the same effective 𝑔-factors are used, VSIMSRG agrees with experiment nearly as well as the shell model. Hence, the wave functions are very similar in both approaches and missing contributions to the M1 operator are identified as the cause of the discrepancy of VS-IMSRG with experiment. Electric quadrupole moments remain more challenging for VS-IMSRG.

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© 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).

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