A study of the indium and germanium photopeaks in the background spectra of Ge spectrometers with a passive shield
Identifieur interne : 000507 ( Main/Exploration ); précédent : 000506; suivant : 000508A study of the indium and germanium photopeaks in the background spectra of Ge spectrometers with a passive shield
Auteurs : RBID : ISTEX:10967_1989_Article_BF02037716.pdfAbstract
Cosmic ray neutron interactions with indium, used as electrical contact within a Ge diode, the diode itself and the surrounding materials can give rise to a large number of photopeaks in the 50 to 1300 keV region of background spectra of Ge spectrometers with a passive shield. The nuclear processes and decays involved in the production of these photopeaks are discussed. These cosmic ray produced photopeaks are compared with those due to primordial radionuclides. Some useful information can be drawn from these measurements on the contribution of the cosmic rays on the background of Ge detectors with a passive shield.
DOI: 10.1007/BF02037716
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<record><TEI><teiHeader><fileDesc><titleStmt><title>A study of the indium and germanium photopeaks in the background spectra of Ge spectrometers with a passive shield</title><author><name>J. -C. Roy</name><affiliation wicri:level="1"><mods:affiliation>Department of Chemistry, Laval University Quebec, G1K 7P4, Quebec, (Canada)</mods:affiliation><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Chemistry, Laval University Quebec, G1K 7P4, Quebec</wicri:regionArea><wicri:noRegion>Quebec</wicri:noRegion></affiliation></author><author><name>J. -E. Côté</name><affiliation wicri:level="1"><mods:affiliation>Department of Chemistry, Laval University Quebec, G1K 7P4, Quebec, (Canada)</mods:affiliation><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Chemistry, Laval University Quebec, G1K 7P4, Quebec</wicri:regionArea><wicri:noRegion>Quebec</wicri:noRegion></affiliation></author><author><name>R. W. Durham</name><affiliation wicri:level="1"><mods:affiliation>Environmental Contaminants Division, National Water Research Institute, Canada Centre for Inland Waters Environment Canada, P.O. Box 5050, L7R 4A6, Burlington, Ontario, (Canada)</mods:affiliation><country xml:lang="fr">Canada</country><wicri:regionArea>Environmental Contaminants Division, National Water Research Institute, Canada Centre for Inland Waters Environment Canada, P.O. Box 5050, L7R 4A6, Burlington, Ontario</wicri:regionArea><wicri:noRegion>Ontario</wicri:noRegion></affiliation></author><author><name>S. R. Joshi</name><affiliation wicri:level="1"><mods:affiliation>Environmental Contaminants Division, National Water Research Institute, Canada Centre for Inland Waters Environment Canada, P.O. Box 5050, L7R 4A6, Burlington, Ontario, (Canada)</mods:affiliation><country xml:lang="fr">Canada</country><wicri:regionArea>Environmental Contaminants Division, National Water Research Institute, Canada Centre for Inland Waters Environment Canada, P.O. Box 5050, L7R 4A6, Burlington, Ontario</wicri:regionArea><wicri:noRegion>Ontario</wicri:noRegion></affiliation></author></titleStmt><publicationStmt><idno type="RBID">ISTEX:10967_1989_Article_BF02037716.pdf</idno><date when="1989">1989</date><idno type="doi">10.1007/BF02037716</idno><idno type="wicri:Area/Main/Corpus">000470</idno><idno type="wicri:Area/Main/Curation">000470</idno><idno type="wicri:Area/Main/Exploration">000507</idno></publicationStmt></fileDesc><profileDesc><textClass></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="eng">Cosmic ray neutron interactions with indium, used as electrical contact within a Ge diode, the diode itself and the surrounding materials can give rise to a large number of photopeaks in the 50 to 1300 keV region of background spectra of Ge spectrometers with a passive shield. The nuclear processes and decays involved in the production of these photopeaks are discussed. These cosmic ray produced photopeaks are compared with those due to primordial radionuclides. Some useful information can be drawn from these measurements on the contribution of the cosmic rays on the background of Ge detectors with a passive shield.</div></front></TEI><mods xsi:schemaLocation="http://www.loc.gov/mods/v3 file:///applis/istex/home/loadistex/home/etc/xsd/mods.xsd" version="3.4" istexId="51a5f251d29120215ffca2b8bd46f4ccedc84eab"><titleInfo lang="eng"><title>A study of the indium and germanium photopeaks in the background spectra of Ge spectrometers with a passive shield</title></titleInfo><name type="personal"><namePart type="given">J. -C.</namePart><namePart type="family">Roy</namePart><role><roleTerm type="text">author</roleTerm></role><affiliation>Department of Chemistry, Laval University Quebec, G1K 7P4, Quebec, (Canada)</affiliation></name><name type="personal"><namePart type="given">J. -E.</namePart><namePart type="family">Côté</namePart><role><roleTerm type="text">author</roleTerm></role><affiliation>Department of Chemistry, Laval University Quebec, G1K 7P4, Quebec, (Canada)</affiliation></name><name type="personal"><namePart type="given">R. W.</namePart><namePart type="family">Durham</namePart><role><roleTerm type="text">author</roleTerm></role><affiliation>Environmental Contaminants Division, National Water Research Institute, Canada Centre for Inland Waters Environment Canada, P.O. Box 5050, L7R 4A6, Burlington, Ontario, (Canada)</affiliation></name><name type="personal"><namePart type="given">S. R.</namePart><namePart type="family">Joshi</namePart><role><roleTerm type="text">author</roleTerm></role><affiliation>Environmental Contaminants Division, National Water Research Institute, Canada Centre for Inland Waters Environment Canada, P.O. Box 5050, L7R 4A6, Burlington, Ontario, (Canada)</affiliation></name><typeOfResource>text</typeOfResource><genre>Original Paper</genre><originInfo><publisher>Kluwer Academic Publishers, Dordrecht</publisher><dateCreated encoding="w3cdtf">1988-07-11</dateCreated><dateValid encoding="w3cdtf">2005-07-20</dateValid><copyrightDate encoding="w3cdtf">1989</copyrightDate></originInfo><language><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType></physicalDescription><abstract lang="eng">Cosmic ray neutron interactions with indium, used as electrical contact within a Ge diode, the diode itself and the surrounding materials can give rise to a large number of photopeaks in the 50 to 1300 keV region of background spectra of Ge spectrometers with a passive shield. The nuclear processes and decays involved in the production of these photopeaks are discussed. These cosmic ray produced photopeaks are compared with those due to primordial radionuclides. Some useful information can be drawn from these measurements on the contribution of the cosmic rays on the background of Ge detectors with a passive shield.</abstract><relatedItem type="series"><titleInfo type="abbreviated"><title>Journal of Radioanalytical and Nuclear Chemistry, Articles</title></titleInfo><titleInfo><title>Journal of Radioanalytical and Nuclear Chemistry</title><subTitle>An International Journal Dealing with All Aspects and Applications of Nuclear Chemistry</subTitle><partNumber>Year: 1989</partNumber><partNumber>Volume: 130</partNumber><partNumber>Number: 1</partNumber></titleInfo><genre>Archive Journal</genre><originInfo><dateIssued encoding="w3cdtf">1989-03-01</dateIssued><copyrightDate encoding="w3cdtf">1989</copyrightDate></originInfo><subject usage="primary"><topic>Chemistry</topic><topic>Inorganic Chemistry</topic><topic>Physical Chemistry</topic><topic>Diagnostic Radiology</topic><topic>Nuclear Physics, Heavy Ions, Hadrons</topic><topic>Nuclear Chemistry</topic></subject><identifier type="issn">0236-5731</identifier><identifier type="issn">Electronic: 1588-2780</identifier><identifier type="matrixNumber">10967</identifier><identifier type="local">IssueArticleCount: 23</identifier><recordInfo><recordOrigin>Akadémiai Kiadó, 1989</recordOrigin></recordInfo></relatedItem><identifier type="doi">10.1007/BF02037716</identifier><identifier type="matrixNumber">Art22</identifier><identifier type="local">BF02037716</identifier><accessCondition type="use and reproduction">MetadataGrant: OpenAccess</accessCondition><accessCondition type="use and reproduction">AbstractGrant: OpenAccess</accessCondition><accessCondition type="restriction on access">BodyPDFGrant: Restricted</accessCondition><accessCondition type="restriction on access">BodyHTMLGrant: Restricted</accessCondition><accessCondition type="restriction on access">BibliographyGrant: Restricted</accessCondition><accessCondition type="restriction on access">ESMGrant: Restricted</accessCondition><part><extent unit="pages"><start>221</start><end>230</end></extent></part><recordInfo><recordOrigin>Akadémiai Kiadó, 1989</recordOrigin><recordIdentifier>10967_1989_Article_BF02037716.pdf</recordIdentifier></recordInfo></mods></record>Pour manipuler ce document sous Unix (Dilib)
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