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The measurement of the (206)Pb(n,gamma) cross section and stellar implications

dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorAbbondanno, U.
dc.contributor.authorAerts, G.
dc.contributor.authorAlvarez, H.
dc.contributor.authorAlvarez-Velarde, F.
dc.contributor.authorAndriamonje, S.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAssimakopoulos, P.
dc.contributor.authorAudouin, L.
dc.contributor.authorBadurek, G.
dc.contributor.authorBaumann, P.
dc.contributor.authorBecvar, F.
dc.contributor.authorBerthoumieux, E.
dc.contributor.authorBisterzo, S.
dc.contributor.authorCalvino, F.
dc.contributor.authorCalviani, M.
dc.contributor.authorCano-Ott, D.
dc.contributor.authorCapote, R.
dc.contributor.authorCarrapico, C.
dc.contributor.authorCennini, P.
dc.contributor.authorChepel, V.
dc.contributor.authorColonna, N.
dc.contributor.authorCortes, G.
dc.contributor.authorCouture, A.
dc.contributor.authorCox, J.
dc.contributor.authorDahlfors, M.
dc.contributor.authorDavid, S.
dc.contributor.authorDillmann, I.
dc.contributor.authorDridi, W.
dc.contributor.authorDuran, I.
dc.contributor.authorEleftheriadis, C.
dc.contributor.authorEmbid-Segura, M.
dc.contributor.authorFerrant, L.
dc.contributor.authorFerrari, A.
dc.contributor.authorFerreira-Marques, R.
dc.contributor.authorFujii, K.
dc.contributor.authorFurman, W.
dc.contributor.authorGallino, R.
dc.contributor.authorGoncalves, I.
dc.contributor.authorGonzalez-Romero, E.
dc.contributor.authorGramegna, F.
dc.contributor.authorGuerrero, C.
dc.contributor.authorGunsing, F.
dc.contributor.authorHaas, B.
dc.contributor.authorHaight, R.
dc.contributor.authorHeil, M.
dc.contributor.authorHerrera-Martinez, A.
dc.contributor.authorIgashira, M.
dc.contributor.authorJericha, E.
dc.contributor.authorKadi, Y.
dc.contributor.authorKaeppeler, F.
dc.contributor.authorKaradimos, D.
dc.contributor.authorKaramanis, D.
dc.contributor.authorKerveno, M.
dc.contributor.authorKoehler, P.
dc.contributor.authorKossionides, E.
dc.contributor.authorKrticka, M.
dc.contributor.authorLamboudis, C.
dc.contributor.authorLeeb, H.
dc.contributor.authorLindote, A.
dc.contributor.authorLopes, I.
dc.contributor.authorLozano, M.
dc.contributor.authorLukic, S.
dc.contributor.authorMarganiec, J.
dc.contributor.authorMarrone, S.
dc.contributor.authorMassimi, C.
dc.contributor.authorMastinu, P.
dc.contributor.authorMengoni, A.
dc.contributor.authorMilazzo, P. M.
dc.contributor.authorMosconi, M.
dc.contributor.authorNeves, F.
dc.contributor.authorOberhummer, H.
dc.contributor.authorO'Brien, S.
dc.contributor.authorPancin, J.
dc.contributor.authorPapachristodoulou, C.
dc.contributor.authorPapadopoulos, C.
dc.contributor.authorParadela, C.
dc.contributor.authorPatronis, N.
dc.contributor.authorPavlik, A.
dc.contributor.authorPavlopoulos, P.
dc.contributor.authorPerrot, L.
dc.contributor.authorPigni, M. T.
dc.contributor.authorPlag, R.
dc.contributor.authorPlompen, A.
dc.contributor.authorPlukis, A.
dc.contributor.authorPoch, A.
dc.contributor.authorPretel, C.
dc.contributor.authorQuesada, J.
dc.contributor.authorRauscher, T.
dc.contributor.authorReifarth, R.
dc.contributor.authorRubbia, C.
dc.contributor.authorRudolf, G.
dc.contributor.authorRullhusen, P.
dc.contributor.authorSalgado, J.
dc.contributor.authorSantos, C.
dc.contributor.authorSarchiapone, L.
dc.contributor.authorSavvidis, I.
dc.contributor.authorStephan, C.
dc.contributor.authorTagliente, G.
dc.contributor.authorTain, J. L.
dc.contributor.authorTassan-Got, L.
dc.contributor.authorTavora, L.
dc.contributor.authorTerlizzi, R.
dc.contributor.authorVannini, G.
dc.contributor.authorVaz, P.
dc.contributor.authorVentura, A.
dc.contributor.authorVillamarin, D.
dc.contributor.authorVincente, M. C.
dc.contributor.authorVlachoudis, V.
dc.contributor.authorVlastou, R.
dc.contributor.authorVoss, F.
dc.contributor.authorWalter, S.
dc.contributor.authorWiescher, M.
dc.contributor.authorWisshak, K.
dc.date.accessioned2013-11-21T12:20:52Z
dc.date.available2013-11-21T12:20:52Z
dc.date.issued2008-01
dc.identifier.citationDomingo-Pardo , C , Abbondanno , U , Aerts , G , Alvarez , H , Alvarez-Velarde , F , Andriamonje , S , Andrzejewski , J , Assimakopoulos , P , Audouin , L , Badurek , G , Baumann , P , Becvar , F , Berthoumieux , E , Bisterzo , S , Calvino , F , Calviani , M , Cano-Ott , D , Capote , R , Carrapico , C , Cennini , P , Chepel , V , Colonna , N , Cortes , G , Couture , A , Cox , J , Dahlfors , M , David , S , Dillmann , I , Dridi , W , Duran , I , Eleftheriadis , C , Embid-Segura , M , Ferrant , L , Ferrari , A , Ferreira-Marques , R , Fujii , K , Furman , W , Gallino , R , Goncalves , I , Gonzalez-Romero , E , Gramegna , F , Guerrero , C , Gunsing , F , Haas , B , Haight , R , Heil , M , Herrera-Martinez , A , Igashira , M , Jericha , E , Kadi , Y , Kaeppeler , F , Karadimos , D , Karamanis , D , Kerveno , M , Koehler , P , Kossionides , E , Krticka , M , Lamboudis , C , Leeb , H , Lindote , A , Lopes , I , Lozano , M , Lukic , S , Marganiec , J , Marrone , S , Massimi , C , Mastinu , P , Mengoni , A , Milazzo , P M , Mosconi , M , Neves , F , Oberhummer , H , O'Brien , S , Pancin , J , Papachristodoulou , C , Papadopoulos , C , Paradela , C , Patronis , N , Pavlik , A , Pavlopoulos , P , Perrot , L , Pigni , M T , Plag , R , Plompen , A , Plukis , A , Poch , A , Pretel , C , Quesada , J , Rauscher , T , Reifarth , R , Rubbia , C , Rudolf , G , Rullhusen , P , Salgado , J , Santos , C , Sarchiapone , L , Savvidis , I , Stephan , C , Tagliente , G , Tain , J L , Tassan-Got , L , Tavora , L , Terlizzi , R , Vannini , G , Vaz , P , Ventura , A , Villamarin , D , Vincente , M C , Vlachoudis , V , Vlastou , R , Voss , F , Walter , S , Wiescher , M & Wisshak , K 2008 , ' The measurement of the (206)Pb(n,gamma) cross section and stellar implications ' , Journal of Physics G: Nuclear and Particle Physics , vol. 35 , no. 1 , 014020 . https://doi.org/10.1088/0954-3899/35/1/014020
dc.identifier.issn0954-3899
dc.identifier.urihttp://hdl.handle.net/2299/12146
dc.description.abstractThe neutron capture cross section of (206)Pb has been measured at the CERN n_TOF spectrometer using a setup of two C(6)D(6) 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 of (206)Pb 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 of (206)Pb is dominated by alpha-back decays of short-lived transbismuth isotopesen
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofJournal of Physics G: Nuclear and Particle Physics
dc.subjectCHRONOMETERS
dc.subjectSTARS
dc.subjectELEMENTS
dc.subjectLEAD
dc.subjectNEUTRON-CAPTURE
dc.subjectGALACTIC CHEMICAL EVOLUTION
dc.titleThe measurement of the (206)Pb(n,gamma) cross section and stellar implicationsen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1088/0954-3899/35/1/014020
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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