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 |
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 |
Dillmann, I |
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 |
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 |
Gramegna, F |
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 |
Jericha, E |
en |
dc.contributor.author |
Kadi, Y |
en |
dc.contributor.author |
Kappeler, F |
en |
dc.contributor.author |
Karadimos, D |
en |
dc.contributor.author |
Karamanis, D |
en |
dc.contributor.author |
Kerveno, M |
en |
dc.contributor.author |
Koehler, P |
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 |
Mosconi, M |
en |
dc.contributor.author |
Neves, F |
en |
dc.contributor.author |
Oberhummer, H |
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 |
Pigni, MT |
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 |
Rubbia, C |
en |
dc.contributor.author |
Rudolf, G |
en |
dc.contributor.author |
Rullhusen, P |
en |
dc.contributor.author |
Salgado, J |
en |
dc.contributor.author |
Santos, C |
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 |
Wiescher, M |
en |
dc.contributor.author |
Wisshak, K |
en |
dc.date.accessioned |
2014-03-01T01:29:20Z |
|
dc.date.available |
2014-03-01T01:29:20Z |
|
dc.date.issued |
2008 |
en |
dc.identifier.issn |
09543899 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/19227 |
|
dc.subject |
Cross Section |
en |
dc.title |
The measurement of the206Pb(n, γ) cross section and stellar implications |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1088/0954-3899/35/1/014020 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/0954-3899/35/1/014020 |
en |
heal.identifier.secondary |
014020 |
en |
heal.publicationDate |
2008 |
en |
heal.abstract |
The neutron capture cross section of206Pb has been measured at the CERN n\TOF spectrometer using a setup of two C6D6 detectors. In the energy interval from 1 eV to 600 keV the cross section is dominated by resonances, which were analyzed via the R-matrix analysis code SAMMY. In the relevant energy ranges for stellar nucleosynthesis, i.e., at thermal energies of kT = 8 keV and kT = 23 keV, the present Maxwellian average cross section differs by 20% and 9% from the recommended values of Bao et al respectively. From the new cross section the s-abundance of206Pb could be reliably determined as 70(4)%. This result is of importance in order to test and constrain r-process abundance calculations in the actinide region, because the r-process portion of206Pb is dominated by α-back decays of short-lived transbismuth isotopes. © 2008 IOP Publishing Ltd. |
en |
heal.journalName |
Journal of Physics G: Nuclear and Particle Physics |
en |
dc.identifier.doi |
10.1088/0954-3899/35/1/014020 |
en |
dc.identifier.volume |
35 |
en |
dc.identifier.issue |
1 |
en |