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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F14%3A10283701%21RIV15-MSM-11320___
rdf:type
skos:Concept n20:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1103/PhysRevC.89.025810
dcterms:description
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. 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.
dcterms:title
Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN
skos:prefLabel
Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN Ni-62(n,gamma) and Ni-63(n,gamma) cross sections measured at the n_TOF facility at CERN
skos:notation
RIV/00216208:11320/14:10283701!RIV15-MSM-11320___
n3:aktivita
n9:I n9:P
n3:aktivity
I, P(LG13031)
n3:cisloPeriodika
2
n3:dodaniDat
n7:2015
n3:domaciTvurceVysledku
n6:6949045 n6:4987020 n6:7876009 n6:1983601
n3:druhVysledku
n18:J
n3:duvernostUdaju
n13:S
n3:entitaPredkladatele
n19:predkladatel
n3:idSjednocenehoVysledku
32659
n3:idVysledku
RIV/00216208:11320/14:10283701
n3:jazykVysledku
n8:eng
n3:klicovaSlova
evolution; nuclear-data; weak component; radiative-capture; galactic enrichment; half-life; massive stars; giant branch stars; thermal-neutron capture; s-process nucleosynthesis
n3:klicoveSlovo
n4:giant%20branch%20stars n4:radiative-capture n4:weak%20component n4:nuclear-data n4:evolution n4:s-process%20nucleosynthesis n4:half-life n4:massive%20stars n4:galactic%20enrichment n4:thermal-neutron%20capture
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[162D5BFC374F]
n3:nazevZdroje
Physical Review C - Nuclear Physics
n3:obor
n16:BG
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
115
n3:projekt
n10:LG13031
n3:rokUplatneniVysledku
n7:2014
n3:svazekPeriodika
89
n3:tvurceVysledku
Dressler, R. Berthoumieux, E. Bosnar, D. Calvino, F. Berthier, B. Krtička, Milan Carrapico, C. Brugger, M. Belloni, F. Andrzejewski, J. Bečvář, František Valenta, Stanislav Kivel, N. Boccone, V. Audouin, L. Andriamonje, S. Schumann, D. Barbagallo, M. Lederer, C. Gunsing, F. Reifarth, R. Colonna, N. Massimi, C. Kaeppeler, F. Altstadt, S. Pignatari, M. Calviani, M. Becares, V. Kroll, Jiří Cano-Ott, D. Billowes, J. Wallner, A. Guerrero, C.
n3:wos
000332175500012
s:issn
0556-2813
s:numberOfPages
12
n12:doi
10.1103/PhysRevC.89.025810
n15:organizacniJednotka
11320