Nuclear physics for the Re/Os clock (Journal article)

Mosconi, M./ Heil, M./ Kappeler, F./ Plag, R./ Mengoni, A./ Fujii, K./ Domingo-Pardo, C./ Aerts, G./ Terlizzi, R./ Gallino, R./ Abbondanno, U./ Alvarez, H./ Alvarez-Velarde, F./ Andriamonje, S./ Andrzejewski, J./ Assimakopoulos, P./ Audouin, L./ Badurek, G./ Baumann, P./ Becvar, F./ Berthoumieux, E./ 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./ Furman, W./ Goncalves, I./ Gonzalez-Romero, E./ Gramegna, F./ Guerrero, C./ Gunsing, F./ Haas, B./ Haight, R./ Herrera-Martinez, A./ Igashira, M./ Jericha, E./ Kadi, Y./ 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./ Milazzo, P. 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./ 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./ Vannini, G./ Vaz, P./ Ventura, A./ Villamarin, D./ Vincente, M. C./ Vlachoudis, V./ Vlastou, R./ Voss, F./ Walter, S./ Wiescher, M./ Wisshak, K./ n TOF Collaboration

Dating the age of the universe by the beta-decay of (187)Re (t(1/2) = 41.2 Gyr) requires the accurate assessment of the s-process reaction flow. The daughter nucleus (187)Os as well as its immediate s-only neighbor (186)Os are shielded from the r-process. Therefore, the radiogenic contribution to (187)Os can be derived via the local approximation of the s-process, which is well justified in this mass region: ( N(s))(187) = ( N(s))(186). Accordingly, accurate Maxwellian-averaged (n,gamma) cross sections have to be known for (186)Os and (187)Os over the full range of s-process temperatures. Because (187)Os has low-lying excited states, which are significantly populated during the s-process, neutron captures on these excited states have to be properly taken into account. The input for the corresponding Hauser-Feshbach calculations can be constrained by deriving the strength functions from a detailed resonance analysis of the measured (n,gamma) cross sections as well as by an additional measurement of the inelastic scattering cross section for the first exited level, which dominates the competition between the capture and scattering channels. This contribution reports on measurements of the neutron capture cross sections of (186)Os, (187)Os and (188)Os from the eV region to 1MeV at the CERN/n_TOF facility and of the inelastic scattering cross section of (187)Os around 30 keV at the Karlsruhe 3.7 MV Van de Graaff accelerator. Based on these results and on a detailed resonance analysis, improved Maxwellian-averaged cross sections were obtained for thermal energies between 5 keV and 100 keV. The implications of these results for the Re/Os clock are discussed.
Institution and School/Department of submitter: Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών
Keywords: neutron cross-sections,inelastic-scattering,nucleosynthesis,os-187,isotopes,stars,age
URI: https://olympias.lib.uoi.gr/jspui/handle/123456789/17501
ISSN: 0954-3899
Link: <Go to ISI>://000252019800016
http://iopscience.iop.org/0954-3899/35/1/014015/pdf/0954-3899_35_1_014015.pdf
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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