dc.creator |
Kanungo, Rituparna |
|
dc.creator |
Prochazka, A. |
|
dc.creator |
Horiuchi, W. |
|
dc.creator |
Nociforo, C. |
|
dc.creator |
Aumann, T. |
|
dc.creator |
Boutin, D. |
|
dc.creator |
Cortina-Gil, D. |
|
dc.creator |
Davids, B. |
|
dc.creator |
Diakaki, M. |
|
dc.creator |
Farinon, F. |
|
dc.creator |
Perro, C. |
|
dc.date.accessioned |
2017-01-13T13:40:08Z |
|
dc.date.available |
2017-01-13T13:40:08Z |
|
dc.date.issued |
2011-02-09 |
|
dc.identifier.issn |
0556-2813 |
|
dc.identifier.uri |
http://library2.smu.ca/handle/01/26730 |
|
dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
The interaction cross sections of [superscript 32–35]Mg at 900A MeV have been measured using the fragment separator at GSI. The deviation from the r[subscript 0]A[superscript 1/3] trend is slightly larger for [superscript 35]Mg, signaling the possible formation of a longer tail in the neutron distribution for [superscript 35]Mg. The radii extracted from a Glauber model analysis with Fermi densities are consistent with models predicting the development of neutron skins. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2017-01-13T13:40:08Z
No. of bitstreams: 1
Kanungo_Rituparna_article_2011_a.pdf: 465077 bytes, checksum: a3110ecf99aef30efdeab9a6980a7c23 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2017-01-13T13:40:08Z (GMT). No. of bitstreams: 1
Kanungo_Rituparna_article_2011_a.pdf: 465077 bytes, checksum: a3110ecf99aef30efdeab9a6980a7c23 (MD5)
Previous issue date: 2011-02-09 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Physical Society |
en_CA |
dc.relation.uri |
https://doi.org/10.1103/PhysRevC.83.021302 |
|
dc.rights |
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user. |
|
dc.subject.lcsh |
Neutrons |
|
dc.subject.lcsh |
Matter |
|
dc.subject.lcsh |
Cross sections (Nuclear physics) |
|
dc.subject.lcsh |
Magnesium -- Isotopes |
|
dc.title |
Matter radii of [superscript 32–35]Mg |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Physical Review C 83, 021302(R). (2011) |
en_CA |
Copyright statement:
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.