dc.creator |
Wilson, G L. |
|
dc.creator |
Catford, W. N. |
|
dc.creator |
Orr, N. A. |
|
dc.creator |
Diget, C. Aa. |
|
dc.creator |
Matta, A. |
|
dc.creator |
Hackman, G. |
|
dc.creator |
Williams, S. J. |
|
dc.creator |
Celik, I. C. |
|
dc.creator |
Achouri, N. L. |
|
dc.creator |
Al Falou, H. |
|
dc.creator |
Austin, Roby Anne Elizabeth, 1974- |
|
dc.creator |
Kanungo, Rituparna |
|
dc.date.accessioned |
2018-02-02T16:05:24Z |
|
dc.date.available |
2018-02-02T16:05:24Z |
|
dc.date.issued |
2016-08-10 |
|
dc.identifier.issn |
0370-2693 |
|
dc.identifier.uri |
http://library2.smu.ca/handle/01/27265 |
|
dc.description |
Publisher's Version/PDF |
|
dc.description.abstract |
The levels in [superscript 26]Na with single particle character have been observed for the first time using the d([superscript 25]Na,p[gamma]) reaction at 5MeV/nucleon. The measured excitation energies and the deduced spectroscopic factors are in good overall agreement with (0 +1)[h bar][omega] shell model calculations performed in a complete spsdf p basis and incorporating a reduction in the N = 20 gap. Notably, the 1p[subscript 3/2] neutron configuration was found to play an enhanced role in the structure of the low-lying negative parity states in [superscript 26]Na, compared to the isotone [superscript 28]Al. Thus, the lowering of the 1p[subscript 3/2] orbital relative to the 0f[subscript 7/2] occurring in the neighbouring Z = 10 and 12 nuclei – [superscript 25,27]Ne and [superscript 27,29]Mg – is seen also to occur at Z = 11 and further strengthens the constraints on the modelling of the transition into the island of inversion. |
en_CA |
dc.description.provenance |
Submitted by Betty McEachern (betty.mceachern@smu.ca) on 2018-02-02T16:05:24Z
No. of bitstreams: 1
Austin_Roby_AE_article_2016.pdf: 1626461 bytes, checksum: a036ec3c8191490941711dfa02542817 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2018-02-02T16:05:24Z (GMT). No. of bitstreams: 1
Austin_Roby_AE_article_2016.pdf: 1626461 bytes, checksum: a036ec3c8191490941711dfa02542817 (MD5)
Previous issue date: 2016 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
Elsevier Science B.V. |
en_CA |
dc.rights |
Creative Commons Attribution License |
|
dc.subject.lcsh |
Nuclear shell theory |
|
dc.subject.lcsh |
Sodium -- Isotopes |
|
dc.subject.lcsh |
Nuclear structure |
|
dc.subject.lcsh |
Radiative transitions |
|
dc.title |
Shell evolution approaching the N = 20 island of inversion: structure of [superscript 26]Na |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Physics Letters B 759, 417-423. (2016) |
en_CA |