dc.creator |
Austin, Roby Anne Elizabeth, 1974- |
|
dc.creator |
Czeszumska, A. |
|
dc.creator |
Angell, C. T. |
|
dc.creator |
Burke, J. T. |
|
dc.creator |
Scielzo, N. D. |
|
dc.creator |
Norman, E. B. |
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dc.creator |
Boutoux, G. |
|
dc.creator |
Casperson, R. J. |
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dc.creator |
Chodash, P. |
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dc.creator |
Hughes, R. O. |
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dc.date.accessioned |
2014-11-21T19:06:36Z |
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dc.date.available |
2014-11-21T19:06:36Z |
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dc.date.issued |
2013-03-12 |
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dc.identifier.issn |
0556-2813 |
|
dc.identifier.issn |
1089-490X |
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dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/25921 |
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dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
Background: Neutron-induced fission cross-section data are needed in various fields of applied and basic nuclear science. However, cross sections of short-lived nuclei are difficult to measure directly due to experimental constraints. Purpose: The first experimental determination of the neutron-induced fission cross section of [superscript 239]Np at nonthermal energies was performed. This minor actinide is the waiting point to [superscript 240]Pu production in a nuclear reactor.
Method: The surrogate ratio method was employed to indirectly deduce the [superscript 239]Np(n, f) cross section. The surrogate reactions used were [superscript 236]U([superscript 3]He, p) and [superscript 238]U([superscript 3]He, p) with the reference cross section given by the well-known [superscript 237]Np(n, f ) cross section. The ratio of observed fission reactions resulting from the two formed compound nuclei, [superscript 238]Np and [superscript 240]Np,was multiplied by the directly measured [superscript 237]Np(n, f ) cross section to determine the [superscript 239]Np(n, f ) cross section. Results: The [superscript 239]Np(n, f ) cross section was determined with an uncertainty ranging between 4% and 30% over the energy range of 0.5–20 MeV. The resulting cross section agrees closest with the JENDL-4.0 evaluation. Conclusions: The measured cross section falls in between the existing evaluations, but it does not match any evaluation exactly (with JENDL-4.0 being the closest match); hence reactor codes relying on existing evaluations may under- or overestimate the amount of [superscript 240]Pu produced during fuel burnup. The measurement helps constrain nuclear structure parameters used in the evaluations. |
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dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2014-11-21T19:06:36Z
No. of bitstreams: 1
Austin_Roby_AE_article_2013.pdf: 822890 bytes, checksum: bff4e0a4efda8908e3bdfd5310204bb1 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2014-11-21T19:06:36Z (GMT). No. of bitstreams: 1
Austin_Roby_AE_article_2013.pdf: 822890 bytes, checksum: bff4e0a4efda8908e3bdfd5310204bb1 (MD5)
Previous issue date: 2013 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Physical Society |
en_CA |
dc.relation.uri |
http://dx.doi.org/10.1103/PhysRevC.87.034613 |
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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. |
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dc.subject.lcsh |
Nuclear fission |
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dc.subject.lcsh |
Nuclear structure |
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dc.subject.lcsh |
Nuclear reactors |
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dc.title |
Determining the [superscript 239]Np(n, f ) cross section using the surrogate ratio method |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Physical Review C 87, 034613. (2013) |
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.