Back to Search Start Over

Shell evolution approaching the N=20 island of inversion: Structure of 29Mg

Authors :
Matta, A.
Catford, W. N.
Orr, N. A.
Henderson, J.
Ruotsalainen, P.
Hackman, G.
Garnsworthy, A. B.
Delaunay, F.
Wilkinson, R.
Lotay, G.
Tsunoda, Naofumi
Otsuka, Takaharu
Knapton, A. J.
Ball, G. C.
Bernier, N.
Burbadge, C.
Chester, A.
Cross, D. S.
Cruz, S.
Diget, C. Aa.
Domingo, T.
Drake, T. E.
Evitts, L. J.
Garcia, F. H.
Hallam, S.
MacConnachie, E.
Moukaddam, M.
Muecher, D.
Padilla-Rodal, E.
Paetkau, O.
Park, J.
Pore, J. L.
Rizwan, U.
Smallcombe, J.
Smith, J. K.
Starosta, K.
Svensson, C. E.
Williams, J.
Williams, M.
Source :
Phys. Rev. C 99, 044320 (2019)
Publication Year :
2019

Abstract

The "Island of Inversion" for neutron-rich nuclei in the vicinity of N=20 has become the testing ground par excellence for our understanding and modelling of shell evolution with isospin. In this context, the structure of the transitional nucleus 29Mg is critical. The first quantitative measurements of the single particle structure of 29Mg are reported, using data from the d(28Mg,p gamma)29Mg reaction. Two key states carrying significant ell=3 (f-wave) strength were identified at 2.40 +/- 0.10 (Jpi = 5/2-) and 4.28 +/- 0.04 MeV (7/2-). New state-of-the-art shell model calculations have been performed and the predictions are compared in detail with the experimental results. Whilst the two lowest 7/2- levels are well described, the sharing of single-particle strength disagrees with experiment for both the 3/2- and 5/2- levels and there appear to be general problems with configurations involving the p3/2 neutron orbital and core-excited components. These conclusions are supported by an analysis of the neutron occupancies in the shell model calculations.<br />Comment: 15 pages, 10 figures, 4 tables

Subjects

Subjects :
Nuclear Experiment

Details

Database :
arXiv
Journal :
Phys. Rev. C 99, 044320 (2019)
Publication Type :
Report
Accession number :
edsarx.1903.12219
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevC.99.044320