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Article: Neutron spectroscopic factors of Ni isotopes from transfer reactions

TitleNeutron spectroscopic factors of Ni isotopes from transfer reactions
Authors
Issue Date2009
Citation
Physical Review C - Nuclear Physics, 2009, v. 79, n. 5 How to Cite?
Abstract177 neutron spectroscopic factors for nickel isotopes have been extracted by performing a systematic analysis of the angular distributions measured from (d,p) transfer reactions. A subset of the extracted spectroscopic factors are compared to predictions of large-basis shell models in the full pf model space using the GXPF1A effective interaction, and the (f5/2,p3/2,p1/2,g9/2) model space using the JJ4PNA interaction. For ground states, the predicted spectroscopic factors using the GXPF1A effective interaction in the full pf model space agree very well with the experimental values, while predictions based on several other effective interactions and model spaces are about 30% higher than the experimental values. For low-energy excited states (<3.5 MeV), the agreement between the extracted spectroscopic factors and shell model calculations is not better than a factor of two. © 2009 The American Physical Society.
Persistent Identifierhttp://hdl.handle.net/10722/199977
ISSN
2014 Impact Factor: 3.733
2015 SCImago Journal Rankings: 1.601
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorLee, Jenny-
dc.contributor.authorTsang, Betty-
dc.contributor.authorLynch, William G.-
dc.contributor.authorHoroi, Mihai-
dc.contributor.authorSu, S. C.-
dc.date.accessioned2014-07-26T23:10:59Z-
dc.date.available2014-07-26T23:10:59Z-
dc.date.issued2009-
dc.identifier.citationPhysical Review C - Nuclear Physics, 2009, v. 79, n. 5-
dc.identifier.issn0556-2813-
dc.identifier.urihttp://hdl.handle.net/10722/199977-
dc.description.abstract177 neutron spectroscopic factors for nickel isotopes have been extracted by performing a systematic analysis of the angular distributions measured from (d,p) transfer reactions. A subset of the extracted spectroscopic factors are compared to predictions of large-basis shell models in the full pf model space using the GXPF1A effective interaction, and the (f5/2,p3/2,p1/2,g9/2) model space using the JJ4PNA interaction. For ground states, the predicted spectroscopic factors using the GXPF1A effective interaction in the full pf model space agree very well with the experimental values, while predictions based on several other effective interactions and model spaces are about 30% higher than the experimental values. For low-energy excited states (<3.5 MeV), the agreement between the extracted spectroscopic factors and shell model calculations is not better than a factor of two. © 2009 The American Physical Society.-
dc.languageeng-
dc.relation.ispartofPhysical Review C - Nuclear Physics-
dc.titleNeutron spectroscopic factors of Ni isotopes from transfer reactions-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1103/PhysRevC.79.054611-
dc.identifier.scopuseid_2-s2.0-66749118459-
dc.identifier.volume79-
dc.identifier.issue5-
dc.identifier.eissn1089-490X-
dc.identifier.isiWOS:000266501700060-

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