Prompt gamma emissions in the reaction 115In(n,gamma)116In for neutrons around the 1.45 eV absorption resonance.
Identifieur interne : 001C95 ( Main/Exploration ); précédent : 001C94; suivant : 001C96Prompt gamma emissions in the reaction 115In(n,gamma)116In for neutrons around the 1.45 eV absorption resonance.
Auteurs : RBID : pubmed:19394840Abstract
The relative intensities of different gamma emissions produced after the reaction (115)In(n,gamma)(116)In were analyzed for the particular case of incident neutron energies around the 1.45 eV indium absorption resonance. For this purpose, a pulsed neutron source in combination with the time-of-flight method for selecting the incident neutron energy range was employed. For neutrons around the mentioned absorption resonance the prompt gamma spectrum was extended to energies below 273 keV, and the intensities of gamma emissions not reported in the literature for epithermal neutrons were determined.
DOI: 10.1016/j.apradiso.2009.03.078
PubMed: 19394840
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For this purpose, a pulsed neutron source in combination with the time-of-flight method for selecting the incident neutron energy range was employed. For neutrons around the mentioned absorption resonance the prompt gamma spectrum was extended to energies below 273 keV, and the intensities of gamma emissions not reported in the literature for epithermal neutrons were determined.</div></front></TEI><pubmed><MedlineCitation Owner="NLM" Status="PubMed-not-MEDLINE"><PMID Version="1">19394840</PMID><DateCreated><Year>2009</Year><Month>06</Month><Day>16</Day></DateCreated><DateCompleted><Year>2009</Year><Month>10</Month><Day>13</Day></DateCompleted><Article PubModel="Print-Electronic"><Journal><ISSN IssnType="Electronic">1872-9800</ISSN><JournalIssue CitedMedium="Internet"><Volume>67</Volume><Issue>9</Issue><PubDate><Year>2009</Year><Month>Sep</Month></PubDate></JournalIssue><Title>Applied radiation and isotopes : including data, instrumentation and methods for use in agriculture, industry and medicine</Title><ISOAbbreviation>Appl Radiat Isot</ISOAbbreviation></Journal><ArticleTitle>Prompt gamma emissions in the reaction 115In(n,gamma)116In for neutrons around the 1.45 eV absorption resonance.</ArticleTitle><Pagination><MedlinePgn>1711-5</MedlinePgn></Pagination><ELocationID EIdType="doi" ValidYN="Y">10.1016/j.apradiso.2009.03.078</ELocationID><Abstract><AbstractText>The relative intensities of different gamma emissions produced after the reaction (115)In(n,gamma)(116)In were analyzed for the particular case of incident neutron energies around the 1.45 eV indium absorption resonance. For this purpose, a pulsed neutron source in combination with the time-of-flight method for selecting the incident neutron energy range was employed. For neutrons around the mentioned absorption resonance the prompt gamma spectrum was extended to energies below 273 keV, and the intensities of gamma emissions not reported in the literature for epithermal neutrons were determined.</AbstractText></Abstract><AuthorList CompleteYN="Y"><Author ValidYN="Y"><LastName>Tartaglione</LastName><ForeName>A</ForeName><Initials>A</Initials><Affiliation>Centro Atómico Bariloche and Instituto Balseiro, GAEN, Comisión Nacional de Energía Atómica, Universidad Nacional de Cuyo, R8402AGP SC de Bariloche, Argentina. tartagla@cab.cnea.gov.ar</Affiliation></Author><Author ValidYN="Y"><LastName>Blostein</LastName><ForeName>J J</ForeName><Initials>JJ</Initials></Author><Author ValidYN="Y"><LastName>Mayer</LastName><ForeName>R E</ForeName><Initials>RE</Initials></Author></AuthorList><Language>eng</Language><PublicationTypeList><PublicationType>Journal Article</PublicationType><PublicationType>Research Support, Non-U.S. Gov't</PublicationType></PublicationTypeList><ArticleDate DateType="Electronic"><Year>2009</Year><Month>04</Month><Day>05</Day></ArticleDate></Article><MedlineJournalInfo><Country>England</Country><MedlineTA>Appl Radiat Isot</MedlineTA><NlmUniqueID>9306253</NlmUniqueID><ISSNLinking>0969-8043</ISSNLinking></MedlineJournalInfo></MedlineCitation><PubmedData><History><PubMedPubDate PubStatus="received"><Year>2008</Year><Month>6</Month><Day>12</Day></PubMedPubDate><PubMedPubDate PubStatus="revised"><Year>2009</Year><Month>2</Month><Day>3</Day></PubMedPubDate><PubMedPubDate PubStatus="accepted"><Year>2009</Year><Month>3</Month><Day>18</Day></PubMedPubDate><PubMedPubDate PubStatus="aheadofprint"><Year>2009</Year><Month>4</Month><Day>5</Day></PubMedPubDate><PubMedPubDate PubStatus="entrez"><Year>2009</Year><Month>4</Month><Day>28</Day><Hour>9</Hour><Minute>0</Minute></PubMedPubDate><PubMedPubDate PubStatus="pubmed"><Year>2009</Year><Month>4</Month><Day>28</Day><Hour>9</Hour><Minute>0</Minute></PubMedPubDate><PubMedPubDate PubStatus="medline"><Year>2009</Year><Month>4</Month><Day>28</Day><Hour>9</Hour><Minute>1</Minute></PubMedPubDate></History><PublicationStatus>ppublish</PublicationStatus><ArticleIdList><ArticleId IdType="pii">S0969-8043(09)00330-3</ArticleId><ArticleId IdType="doi">10.1016/j.apradiso.2009.03.078</ArticleId><ArticleId IdType="pubmed">19394840</ArticleId></ArticleIdList></PubmedData></pubmed></record>Pour manipuler ce document sous Unix (Dilib)
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