Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session DD: Mini-Symposium: The Structural Diversity of Nuclei in the Proximity of N=20 and 28 I
9:00 AM–11:30 AM,
Thursday, October 25, 2018
Hilton
Room: Kohala 3
Chair: Daniel Bazin, Michigan State University
Abstract ID: BAPS.2018.HAW.DD.1
Abstract: DD.00001 : Exotic Isotopes of Magnesium*
9:00 AM–9:30 AM
Presenter:
Heather L Crawford
(Lawrence Berkeley Natl Lab)
Author:
Heather L Crawford
(Lawrence Berkeley Natl Lab)
The structure of nuclei in the vicinity of expected nuclear shell closures away from stability has been, and continues to be, a cornerstone for nuclear structure study. The confirmation of certain ‘magic numbers’ in exotic nuclei provides insight into the evolution of nucleon configurations with isospin, but perhaps even more light is shed into the structure of the atomic nucleus when expected shell closures are found to be weakened, or entirely disappear. The competition between monopole shifts of single particle energies and pairing plus quadrupole correlations leads to competition between spherical and deformed configurations. Around 32Mg the change in effective single particle spacing reduces the N=20 shell gap and the deformed intruder configuration, with neutron pairs promoted from the sd to the fp shell, is energetically favoured. Recent experimental work in the Mg isotopes has suggested a chain of prolate-deformed nuclei along Z=12, extending to N=28 and 40Mg, where there is a similar development of deformation along the isotonic chain below 48Ca, with the removal of protons driving rapid shape oscillations between the N=28 nuclei.
I will give an overview of our knowledge in this part of the nuclear landscape, and discuss the latest experimental results in this region between N=20 and N=28, focusing on the Mg isotopes, and the evolution of their structure with spin, isospin and binding energy.
*This material is based upon work supported by the U.S. DOE, Office of Science, Office of Nuclear Physics under Contract No. DE-AC02-05CH11231.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.DD.1
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