Abstract

Many-body nuclear theory utilizing microscopic or chiral potentials has developed to the point that collectivity might be studied within a microscopic or ab initio framework without the use of effective charges; for example with the proper evolution of the E2 operator, or alternatively, through the use of an appropriate and manageable subset of particle–hole excitations. We present a precise determination of E2 strength in 22Mg and its mirror 22Ne by Coulomb excitation, allowing for rigorous comparisons with theory. No-core symplectic shell-model calculations were performed and agree with the new B(E2) values while in-medium similarity-renormalization-group calculations consistently underpredict the absolute strength, with the missing strength found to have both isoscalar and isovector components. The discrepancy between two microscopic models demonstrates the sensitivity of E2 strength to the choice of many-body approximation employed.

Highlights

  • Recent developments in many-body nuclear theory have seen a great advance in the number of nuclei accessible to microscopically derived theoretical models – including those constructed in an ab initio framework [1,2,3,4,5,6,7,8,9,10,11,12,13,14,15]

  • The first-excited 2+ states in 22Mg and its stable mirror 22Ne were populated through Coulomb excitation in normal kinematics at the TRIUMF-ISAC-II facility. 22Mg was produced using a 50 μA, 480-MeV proton beam impinged on a SiC target coupled to an ion guide laser ion source (IG-LIS) [30,31]

  • B(E2)ETxzp=+1, B ( E 2)TThz =eo+ry1 (1). This analysis was performed for both in-medium similarity-renormalization-group (IM-SRG) and shell-model calculations and the projected B(E2) values were compared with experiment

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Summary

Introduction

Recent developments in many-body nuclear theory have seen a great advance in the number of nuclei accessible to microscopically derived theoretical models – including those constructed in an ab initio framework [1,2,3,4,5,6,7,8,9,10,11,12,13,14,15] As these models increasingly reach regions of the nuclear landscape inaccessible to experiment, it is essential that their performance is scrutinized in detail using less-exotic systems where high-precision experimental data.

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