Journal
PHYSICAL REVIEW C
Volume 82, Issue 3, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.82.034305
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Funding
- US Department of Energy, Office of Nuclear Physics [DE-AC02-06CH11357]
- UK Science and Technology Facilities Council
- US National Science Foundation [PHY-01-01253, PHY-0456463, PHY-07-56474]
- Scottish Universities Physics Alliance
- RIKEN
- Science and Technology Facilities Council [EP/C51646X/1, EP/C516478/1, ST/F008805/1, ST/F012071/1, PP/F000944/1] Funding Source: researchfish
- STFC [EP/C516478/1, ST/F012071/1, PP/F000944/1, ST/F008805/1] Funding Source: UKRI
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Excited states in Mg-30 have been populated to similar to 6 (h) over bar and 5MeV excitation energy with the C-14(O-18, 2p) reaction. Firm spin assignments for states with J > 2 (h) over bar h have been made in this nucleus. The level scheme is compared to shell-model calculations using the Universal sd effective interaction and the Monte Carlo shell model method. Calculations employing a full sd model space fail to reproduce the observed levels. The results indicate that excitations across the N = 20 gap are required at relatively low excitation energy to achieve a description of the data. The incorporation of the f(7/2) and p(3/2) orbitals into the model space gives improved results but indicate the need for further refinement of the models to reproduce the observed spectra.
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