. "Dressler, R." . "Berthoumieux, E." . "Bosnar, D." . "The cross section of the Ni-62(n,gamma) reaction was measured with the time-of-flight technique at the neutron time-of-flight facility n_TOF 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 Ni-63(n,gamma) reaction was measured for the first time at n_TOF. 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." . "Calvino, F." . "Berthier, B." . "Krti\u010Dka, Milan" . "Carrapico, C." . "I, P(LG13031)" . "evolution; nuclear-data; weak component; radiative-capture; galactic enrichment; half-life; massive stars; giant branch stars; thermal-neutron capture; s-process nucleosynthesis"@en . . "Brugger, M." . "Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN"@en . . . . . . . "Belloni, F." . "2" . "115"^^ . "Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN"@en . . "Andrzejewski, J." . . "Be\u010Dv\u00E1\u0159, Franti\u0161ek" . "Valenta, Stanislav" . "Kivel, N." . "Boccone, V." . "10.1103/PhysRevC.89.025810" . "Audouin, L." . "Andriamonje, S." . "Schumann, D." . "Barbagallo, M." . . "Lederer, C." . . "Gunsing, F." . . . "12"^^ . "11320" . . . "Physical Review C - Nuclear Physics" . "Reifarth, R." . . "RIV/00216208:11320/14:10283701" . . . "[162D5BFC374F]" . "Colonna, N." . . . "Massimi, C." . "89" . "Kaeppeler, F." . "Altstadt, S." . "0556-2813" . "32659" . "Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN" . "Pignatari, M." . "000332175500012" . "US - Spojen\u00E9 st\u00E1ty americk\u00E9" . "http://dx.doi.org/10.1103/PhysRevC.89.025810" . . . "Calviani, M." . . "Becares, V." . . "Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN" . "Kroll, Ji\u0159\u00ED" . "Cano-Ott, D." . "Billowes, J." . "The cross section of the Ni-62(n,gamma) reaction was measured with the time-of-flight technique at the neutron time-of-flight facility n_TOF 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 Ni-63(n,gamma) reaction was measured for the first time at n_TOF. 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."@en . "4"^^ . "Wallner, A." . "RIV/00216208:11320/14:10283701!RIV15-MSM-11320___" . "Guerrero, C." . .