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Resonance capture cross section of Pb207

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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 Bisterzo, S en
dc.contributor.author Calvino, F en
dc.contributor.author Cano-Ott, D en
dc.contributor.author Capote, R en
dc.contributor.author Carrapico, C 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 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 2014-03-01T01:25:04Z
dc.date.available 2014-03-01T01:25:04Z
dc.date.issued 2006 en
dc.identifier.issn 0556-2813 en
dc.identifier.uri http://hdl.handle.net/123456789/17532
dc.subject.classification Physics, Nuclear en
dc.subject.other GALACTIC CHEMICAL EVOLUTION en
dc.subject.other GIANT BRANCH STARS en
dc.subject.other NEUTRON-CAPTURE en
dc.subject.other ABUNDANCES en
dc.subject.other ELEMENTS en
dc.subject.other SOLAR en
dc.subject.other NUCLEOSYNTHESIS en
dc.subject.other CHRONOMETERS en
dc.title Resonance capture cross section of Pb207 en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevC.74.055802 en
heal.identifier.secondary 055802 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevC.74.055802 en
heal.language English en
heal.publicationDate 2006 en
heal.abstract The radiative neutron capture cross section of Pb207 has been measured at the CERN neutron time of flight installation n_TOF using the pulse height weighting technique in the resolved energy region. The measurement has been performed with an optimized setup of two C6D6 scintillation detectors, which allowed us to reduce scattered neutron backgrounds down to a negligible level. Resonance parameters and radiative kernels have been determined for 16 resonances by means of an R-matrix analysis in the neutron energy range from 3 keV to 320 keV. Good agreement with previous measurements was found at low neutron energies, whereas substantial discrepancies appear beyond 45 keV. With the present results, we obtain an s-process contribution of 77±8% to the solar abundance of Pb207. This corresponds to an r-process component of 23±8%, which is important for deriving the U/Th ages of metal poor halo stars. © 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.74.055802 en
dc.identifier.isi ISI:000242409500056 en
dc.identifier.volume 74 en
dc.identifier.issue 5 en


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