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New measurement of neutron capture resonances in Bi209

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dc.contributor.author Domingo-Pardo, C en
dc.contributor.author Abbondanno, U en
dc.contributor.author Aerts, G en
dc.contributor.author Alvarez-Pol, H en
dc.contributor.author Alvarez-Velarde, F en
dc.contributor.author Andriamonje, S en
dc.contributor.author Andrzejewski, J en
dc.contributor.author Assimakopoulos, P en
dc.contributor.author Audouin, L en
dc.contributor.author Badurek, G en
dc.contributor.author Baumann, P en
dc.contributor.author Becvar, F en
dc.contributor.author Berthoumieux, E en
dc.contributor.author Calvino, F en
dc.contributor.author Cano-Ott, D en
dc.contributor.author Capote, R en
dc.contributor.author Albornoz, ACD en
dc.contributor.author Cennini, P en
dc.contributor.author Chepel, V en
dc.contributor.author Chiaveri, E en
dc.contributor.author Colonna, N en
dc.contributor.author Cortes, G en
dc.contributor.author Couture, A en
dc.contributor.author Cox, J en
dc.contributor.author Dahlfors, M en
dc.contributor.author David, S en
dc.contributor.author Dillman, I en
dc.contributor.author Dolfini, R en
dc.contributor.author Dridi, W en
dc.contributor.author Duran, I en
dc.contributor.author Eleftheriadis, C en
dc.contributor.author Embid-Segura, M en
dc.contributor.author Ferrant, L en
dc.contributor.author Ferrari, A en
dc.contributor.author Ferreira-Marques, R en
dc.contributor.author Fitzpatrick, L en
dc.contributor.author Frais-Koelbl, H en
dc.contributor.author Fujii, K en
dc.contributor.author Furman, W en
dc.contributor.author Gallino, R en
dc.contributor.author Goncalves, I en
dc.contributor.author Gonzalez-Romero, E en
dc.contributor.author Goverdovski, A en
dc.contributor.author Gramegna, F en
dc.contributor.author Griesmayer, E en
dc.contributor.author Guerrero, C en
dc.contributor.author Gunsing, F en
dc.contributor.author Haas, B en
dc.contributor.author Haight, R en
dc.contributor.author Heil, M en
dc.contributor.author Herrera-Martinez, A en
dc.contributor.author Igashira, M en
dc.contributor.author Isaev, S en
dc.contributor.author Jericha, E en
dc.contributor.author Kadi, Y en
dc.contributor.author Kappeler, F en
dc.contributor.author Karamanis, D en
dc.contributor.author Karadimos, D en
dc.contributor.author Kerveno, M en
dc.contributor.author Ketlerov, V en
dc.contributor.author Koehler, P en
dc.contributor.author Konovalov, V en
dc.contributor.author Kossionides, E en
dc.contributor.author Krticka, M en
dc.contributor.author Lamboudis, C en
dc.contributor.author Leeb, H en
dc.contributor.author Lindote, A en
dc.contributor.author Lopes, I en
dc.contributor.author Lozano, M en
dc.contributor.author Lukic, S en
dc.contributor.author Marganiec, J en
dc.contributor.author Marques, L en
dc.contributor.author Marrone, S en
dc.contributor.author Mastinu, P en
dc.contributor.author Mengoni, A en
dc.contributor.author Milazzo, PM en
dc.contributor.author Moreau, C en
dc.contributor.author Mosconi, M en
dc.contributor.author Neves, F en
dc.contributor.author Oberhummer, H en
dc.contributor.author Oshima, M en
dc.contributor.author O'Brien, S en
dc.contributor.author Pancin, J en
dc.contributor.author Papachristodoulou, C en
dc.contributor.author Papadopoulos, C en
dc.contributor.author Paradela, C en
dc.contributor.author Patronis, N en
dc.contributor.author Pavlik, A en
dc.contributor.author Pavlopoulos, P en
dc.contributor.author Perrot, L en
dc.contributor.author Plag, R en
dc.contributor.author Plompen, A en
dc.contributor.author Plukis, A en
dc.contributor.author Poch, A en
dc.contributor.author Pretel, C en
dc.contributor.author Quesada, J en
dc.contributor.author Rauscher, T en
dc.contributor.author Reifarth, R en
dc.contributor.author Rosetti, M en
dc.contributor.author Rubbia, C en
dc.contributor.author Rudolf, G en
dc.contributor.author Rullhusen, P en
dc.contributor.author Salgado, J en
dc.contributor.author Sarchiapone, L en
dc.contributor.author Savvidis, I en
dc.contributor.author Stephan, C en
dc.contributor.author Tagliente, G en
dc.contributor.author Tain, JL en
dc.contributor.author Tassan-Got, L en
dc.contributor.author Tavora, L en
dc.contributor.author Terlizzi, R en
dc.contributor.author Vannini, G en
dc.contributor.author Vaz, P en
dc.contributor.author Ventura, A en
dc.contributor.author Villamarin, D en
dc.contributor.author Vincente, MC en
dc.contributor.author Vlachoudis, V en
dc.contributor.author Vlastou, R en
dc.contributor.author Voss, F en
dc.contributor.author Walter, S en
dc.contributor.author Wendler, H en
dc.contributor.author Wiescher, M en
dc.contributor.author Wisshak, K en
dc.date.accessioned 2014-03-01T01:24:43Z
dc.date.available 2014-03-01T01:24:43Z
dc.date.issued 2006 en
dc.identifier.issn 0556-2813 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/17410
dc.subject.classification Physics, Nuclear en
dc.subject.other GALACTIC CHEMICAL EVOLUTION en
dc.subject.other CROSS-SECTION en
dc.subject.other S-PROCESS en
dc.subject.other CHRONOMETERS en
dc.subject.other ABUNDANCES en
dc.subject.other FACILITY en
dc.subject.other DETECTOR en
dc.subject.other ELEMENTS en
dc.subject.other SYSTEM en
dc.subject.other STARS en
dc.title New measurement of neutron capture resonances in Bi209 en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevC.74.025807 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevC.74.025807 en
heal.identifier.secondary 025807 en
heal.language English en
heal.publicationDate 2006 en
heal.abstract The neutron capture cross section of Bi209 has been measured at the CERN n_TOF facility by employing the pulse-height-weighting technique. Improvements over previous measurements are mainly because of an optimized detection system, which led to a practically negligible neutron sensitivity. Additional experimental sources of systematic error, such as the electronic threshold in the detectors, summing of γ-rays, internal electron conversion, and the isomeric state in bismuth, have been taken into account. γ-Ray absorption effects inside the sample have been corrected by employing a nonpolynomial weighting function. Because Bi209 is the last stable isotope in the reaction path of the stellar s-process, the Maxwellian averaged capture cross section is important for the recycling of the reaction flow by α decays. In the relevant stellar range of thermal energies between kT=5 and 8 keV our new capture rate is about 16% higher than the presently accepted value used for nucleosynthesis calculations. At this low temperature an important part of the heavy Pb-Bi isotopes are supposed to be synthesized by the s-process in the He shells of low mass, thermally pulsing asymptotic giant branch stars. With the improved set of cross sections we obtain an s-process fraction of 19±3% of the solar bismuth abundance, resulting in an r-process residual of 81±3%. The present (n,γ) cross-section measurement is also of relevance for the design of accelerator driven systems based on a liquid metal Pb/Bi spallation target. © 2006 The American Physical Society. en
heal.publisher AMERICAN PHYSICAL SOC en
heal.journalName Physical Review C - Nuclear Physics en
dc.identifier.doi 10.1103/PhysRevC.74.025807 en
dc.identifier.isi ISI:000240239100068 en
dc.identifier.volume 74 en
dc.identifier.issue 2 en


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