dc.creator |
Kanungo, Rituparna |
|
dc.creator |
Tanihata, I. |
|
dc.creator |
Ozawa, A. |
|
dc.date.accessioned |
2015-10-05T15:46:04Z |
|
dc.date.available |
2015-10-05T15:46:04Z |
|
dc.date.issued |
2001-07-19 |
|
dc.identifier.issn |
0370-2693 |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/26381 |
|
dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
The recently measured interaction cross section data for [superscript 22]N, [superscript 23]O, and [superscript 24]F in a [superscript 12]C target at relativistic energies have been analysed in a few body Glauber model approach. Conventional fixed core-plus-neutron model for halo nuclei is unable to explain the observed enhanced cross section for these nuclei by any selection of the neutron orbitals. Microscopic calculations like many-body Monte Carlo shell model, relativistic mean field theory and cluster model are also shown to fail in describing the large difference if interaction cross section between [superscript 22]O and [superscript 23]O. A possibility of core enlargement is suggested in these nuclei. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2015-10-05T15:46:04Z
No. of bitstreams: 1
Kanungo_Rituparna_article_2001.pdf: 241872 bytes, checksum: 4dad4e1132a4502b2a16f112b6934156 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2015-10-05T15:46:04Z (GMT). No. of bitstreams: 1
Kanungo_Rituparna_article_2001.pdf: 241872 bytes, checksum: 4dad4e1132a4502b2a16f112b6934156 (MD5)
Previous issue date: 2001-07-19 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
Elsevier |
en_CA |
dc.title |
Possibility of enlarged core structure of N = 15 neutron-rich nuclei |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Physics Letters B 512, 261-267. (2001) |
en_CA |