⁶²Ni(n,γ) and ⁶³Ni(n,γ) cross sections measured at nₜOF/CERN
Lederer, C. · Massimi, C. · Berthoumieux, E. · Colonna, N. · Dressler, R. · Guerrero, C. · Gunsing, F. · Käppeler, F. · Kivel, N. · Pignatari, M. · Reifarth, R. · Schumann, D. · Wallner, A. · Altstadt, S. · Andriamonje, S. · Andrzejewski, J. · Audouin, L. · Barbagallo, M. · Becares, V. · Becvar, F. · Belloni, F. · Berthier, B. · Billowes, J. · Boccone, V. · Bosnar, D. · Brugger, M. · Calviani, M. · Calvino, F. · Cano-Ott, D. · Carrapico, C. · Cerutti, F. · Chiaveri, E. · Chin, M. · Cortes, G. · Cortes-Giraldo, M. A. · Dillmann, I. · Domingo-Pardo, C. · Duran, I. · Dzysiuk, N. · Eleftheriadis, C. · Fernandez-Ordonez, M. · Ferrari, A. · Fraval, K. · Ganesan, S. · Garcıa, A. R. · Giubrone, G. · Gomez-Hornillos, M. B. · Goncalves, I. F. · Gonzalez-Romero, E. · Gramegna, F. · Griesmayer, E. · Gurusamy, P. · Harrisopulos, S. · Heil, M. · Ioannides, K. · Jenkins, D. G. · Jericha, E. · Kadi, Y. · Karadimos, D. · Korschinek, G. · Krticka, M. · Kroll, J. · Langer, C. · Lebbos, E. · Leeb, H. · Leong, L. S. · Losito, R. · Lozano, M. · Manousos, A. · Marganiec, J. · Marrone, S. · Martinez, T. · Mastinu, P. F. · Mastromarco, M. · Meaze, M. · Mendoza, E. · Mengoni, A. · Milazzo, P. M. · Mingrone, F. · Mirea, M. · Mondalaers, W. · Paradela, C. · Pavlik, A. · Perkowski, J. · Plag, R. · Plompen, A. · Praena, J. · Quesada, J. M. · Rauscher, T. · Riego, A. · Roman, F. · Rubbia, C. · Sarmento, R. · Schillebeeckx, P. · Schmidt, S. · Tagliente, G. · Tain, J. L. · Tarrıo, D. · Tassan-Got, L. · Tsinganis, A. · Tlustos, L. · Valenta, S. · Vannini, G. · Variale, V. · Vaz, P. · Ventura, A. · Vermeulen, M. J. · Versaci, R. · Vlachoudis, V. · Vlastou, R. · Ware, T. · Weigand, M. · Weiß, C. · Wright, T. J. · Zugec, P.
Original · EN
The cross section of the ⁶²Ni(n,γ) reaction was measured with the time-of-flight technique at the neutron time-of-flight facility nₜOF at CERN. Capture kernels of 42 resonances were analyzed up to 200 keV neutron energy and Maxwellian averaged cross sections (MACS) from kT=5-100 keV were calculated. With a total uncertainty of 4.5%, the stellar cross section is in excellent agreement with the the KADoNiS compilation at kT=30 keV, while being systematically lower up to a factor of 1.6 at higher stellar temperatures. The cross section of the ⁶³Ni(n,γ) reaction was measured for the first time at nₜOF. We determined unresolved cross sections from 10 to 270 keV with a systematic uncertainty of 17%. These results provide fundamental constraints on s-process production of heavier species, especially the production of Cu in massive stars, which serve as the dominant source of Cu in the solar system.
English translation
This paper has no Arabic translation yet. Be the first: it takes a few seconds, and the result is stored for every future reader.