Possibility of enlarged core structure of N = 15 neutron-rich nuclei

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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.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


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