$^{92}$Zr($n,\gamma$) and ($n$,tot) measurements at the GELINA and n_TOF facilities

Background: Stellar nucleosynthesis of elements heavier than iron is driven by neutron capture processes. 92Zr is positioned at a strategic point along the slow nucleosynthesis path, given its proximity to the neutron magic number N = 50 and its position at the matching region between the weak and m...

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Detalles Bibliográficos
Autores principales: Tagliente, G, Kopecky, S, Heyse, J, Krtička, M, Massimi, C, Mengoni, A, Milazzo, P M, Plompen, A J M, Schillebeeckx, P, Valenta, S, Wynants, R, Altstadt, S, Andrzejewski, J, Audouin, L, Bécares, V, Barbagallo, M, Bečvář, F, Belloni, F, Berthoumieux, E, Billowes, J, Boccone, V, Bosnar, D, Brugger, M, Calviño, F, Calviani, M, Cano-Ott, D, Carrapiço, C, Cerutti, F, Chiaveri, E, Chin, M, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Cristallo, S, Diakaki, M, Domingo-Pardo, C, Dressler, R, Durán, I, Eleftheriadis, C, Ferrari, A, Fraval, K, Furman, V, Göbel, K, Gómez-Hornillos, M B, Ganesan, S, García, A R, Giubrone, G, Gonçalves, I F, González-Romero, E, Goverdovski, A, Griesmayer, E, Guerrero, C, Gunsing, F, Heftrich, T, Hernández-Prieto, A, Jericha, E, Käppeler, F, Kadi, Y, Karadimos, D, Katabuchi, T, Ketlerov, V, Khryachkov, V, Kivel, N, Kokkoris, M, Kroll, J, Lampoudis, C, Langer, C, Leal-Cidoncha, E, Lederer, C, Leeb, H, Leong, L S, Losito, R, Lugaro, M, Mallick, A, Manousos, A, Marganiec, J, Martínez, T, Mastinu, P, Mastromarco, M, Mendoza, E, Mingrone, F, Mirea, M, Paradela, C, Pavlik, A, Perkowski, J, Praena, J, Quesada, J M, Rauscher, T, Reifarth, R, Riego-Perez, A, Robles, M, Rubbia, C, Ryan, J A, Sabaté-Gilarte, M, Sarmento, R, Saxena, A, Schmidt, S, Schumann, D, Sedyshev, P, Tain, J L, Tarifeño-Saldivia, A, Tarrío, D, Tassan-Got, L, Tsinganis, A, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vermeulen, M J, Vescovi, D, Vlachoudis, V, Vlastou, R, Wallner, A, Ware, T, Weigand, M, Weiss, C, Wright, T, Žugec, P
Lenguaje:eng
Publicado: 2022
Materias:
Nuclear Physics - Experiment
Acceso en línea:https://dx.doi.org/10.1103/PhysRevC.105.025805
http://cds.cern.ch/record/2806079

Internet

https://dx.doi.org/10.1103/PhysRevC.105.025805
http://cds.cern.ch/record/2806079

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