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Measurement of the radiative neutron capture cross section of Pb206 and its astrophysical implications

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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, 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 Calviani, M 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, M en
dc.contributor.author Jericha, E en
dc.contributor.author Kappeler, F en
dc.contributor.author Kadi, Y en
dc.contributor.author Karadimos, D en
dc.contributor.author Karamanis, 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 Massimi, C 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 2014-03-01T01:56:20Z
dc.date.available 2014-03-01T01:56:20Z
dc.date.issued 2007 en
dc.identifier.issn 05562813 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/28065
dc.title Measurement of the radiative neutron capture cross section of Pb206 and its astrophysical implications en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevC.76.045805 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevC.76.045805 en
heal.identifier.secondary 045805 en
heal.publicationDate 2007 en
heal.abstract The (n,γ) cross section of Pb206 has been measured at the CERN n_TOF facility with high resolution in the energy range from 1 eV to 620 keV by using two optimized C6D6 detectors. In the investigated energy interval about 130 resonances could be observed, from which 61 had enough statistics to be reliably analyzed via the R-matrix analysis code SAMMY. Experimental uncertainties were minimized, in particular with respect to (i) angular distribution effects of the prompt capture γ-rays, and to (ii) the TOF-dependent background due to sample-scattered neutrons. Other background components were addressed by background measurements with an enriched Pb208 sample. The effect of the lower energy cutoff in the pulse height spectra of the C6D6 detectors was carefully corrected via Monte Carlo simulations. Compared to previous Pb206 values, the Maxwellian averaged capture cross sections derived from these data are about 20% and 9% lower at thermal energies of 5 keV and 30 keV, respectively. These new results have a direct impact on the s-process abundance of Pb206, which represents an important test for the interpretation of the cosmic clock based on the decay of U238. © 2007 The American Physical Society. en
heal.journalName Physical Review C - Nuclear Physics en
dc.identifier.doi 10.1103/PhysRevC.76.045805 en
dc.identifier.volume 76 en
dc.identifier.issue 4 en


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