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dc.contributor.authorVERMOTE S.en_GB
dc.contributor.authorWagemans C.en_GB
dc.contributor.authorDE SMET L.en_GB
dc.contributor.authorLAMPOUDIS C.en_GB
dc.contributor.authorVAN GILS J.en_GB
dc.date.accessioned2012-05-08T00:01:35Z-
dc.date.available2012-05-07en_GB
dc.date.available2012-05-08T00:01:35Z-
dc.date.created2012-04-12en_GB
dc.date.issued2012en_GB
dc.date.submitted2012-03-23en_GB
dc.identifier.citationPHYSICAL REVIEW C vol. 85 no. 1 p. 015803 (1-8)en_GB
dc.identifier.issn0556-2813en_GB
dc.identifier.urihttp://prc.aps.org/abstract/PRC/v85/i1/e015803en_GB
dc.identifier.urihttp://publications.jrc.ec.europa.eu/repository/handle/JRC69977-
dc.description.abstractThe 41Ca(n,α)38Ar reaction cross section was studied at the linear accelerator GELINA of the Institute for Reference Materials and Measurements in Geel (Belgium) and was determined up to a neutron energy of about 80 keV using the time-of-flight technique. In this energy region, 15 resonances were observed, whereas none were identified before. For some of them, resonance parameters such as resonance energy, total width, area, and spin could be determined. From the obtained cross-section data, Maxwellian average cross sections have been calculated at various stellar temperatures for further use in stellar models.en_GB
dc.description.sponsorshipJRC.D.4-Nuclear physicsen_GB
dc.format.mediumPrinteden_GB
dc.languageENGen_GB
dc.publisherAMER PHYSICAL SOCen_GB
dc.relation.ispartofseriesJRC69977en_GB
dc.titleExperimental determination of the 41Ca(n,α)38Ar reaction cross section up to 80 keV, and calculation of the Maxwellian averaged cross section at stellar temperaturesen_GB
dc.typeArticles in periodicals and booksen_GB
dc.identifier.doi10.1103/PhysRevC.85.015803en_GB
JRC Directorate:Health, Consumers and Reference Materials

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