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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F13%3A10159449%21RIV14-MSM-11320___
rdf:type
skos:Concept n11:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1103/PhysRevLett.110.022501
dcterms:description
The Ni-63(n, gamma) cross section has been measured for the first time at the neutron time-of-flight facility n_TOF at CERN from thermal neutron energies up to 200 keV. In total, capture kernels of 12 (new) resonances were determined. Maxwellian averaged cross sections were calculated for thermal energies from kT = 5-100 keV with uncertainties around 20%. Stellar model calculations for a 25M(circle dot) star show that the new data have a significant effect on the s-process production of Cu-63, Ni-64, and Zn-64 in massive stars, allowing stronger constraints on the Cu yields from explosive nucleosynthesis in the subsequent supernova. DOI: 10.1103/PhysRevLett.110.022501 The Ni-63(n, gamma) cross section has been measured for the first time at the neutron time-of-flight facility n_TOF at CERN from thermal neutron energies up to 200 keV. In total, capture kernels of 12 (new) resonances were determined. Maxwellian averaged cross sections were calculated for thermal energies from kT = 5-100 keV with uncertainties around 20%. Stellar model calculations for a 25M(circle dot) star show that the new data have a significant effect on the s-process production of Cu-63, Ni-64, and Zn-64 in massive stars, allowing stronger constraints on the Cu yields from explosive nucleosynthesis in the subsequent supernova. DOI: 10.1103/PhysRevLett.110.022501
dcterms:title
Neutron Capture Cross Section of Unstable Ni-63: Implications for Stellar Nucleosynthesis Neutron Capture Cross Section of Unstable Ni-63: Implications for Stellar Nucleosynthesis
skos:prefLabel
Neutron Capture Cross Section of Unstable Ni-63: Implications for Stellar Nucleosynthesis Neutron Capture Cross Section of Unstable Ni-63: Implications for Stellar Nucleosynthesis
skos:notation
RIV/00216208:11320/13:10159449!RIV14-MSM-11320___
n11:predkladatel
n14:orjk%3A11320
n3:aktivita
n10:Z n10:I
n3:aktivity
I, Z(MSM0021620859)
n3:cisloPeriodika
2
n3:dodaniDat
n16:2014
n3:domaciTvurceVysledku
n5:7876009 n5:6949045 n5:1983601 n5:4987020
n3:druhVysledku
n4:J
n3:duvernostUdaju
n17:S
n3:entitaPredkladatele
n15:predkladatel
n3:idSjednocenehoVysledku
91490
n3:idVysledku
RIV/00216208:11320/13:10159449
n3:jazykVysledku
n12:eng
n3:klicovaSlova
uncertainties; standardization; rates; nuclear; half-life; weak component; statistical-model; model calculations; massive stars; s-process nucleosynthesis
n3:klicoveSlovo
n7:model%20calculations n7:standardization n7:half-life n7:rates n7:s-process%20nucleosynthesis n7:statistical-model n7:massive%20stars n7:weak%20component n7:nuclear n7:uncertainties
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[2EDE2B814A14]
n3:nazevZdroje
Physical Review Letters
n3:obor
n21:BG
n3:pocetDomacichTvurcuVysledku
4
n3:pocetTvurcuVysledku
105
n3:rokUplatneniVysledku
n16:2013
n3:svazekPeriodika
110
n3:tvurceVysledku
Cortes-Giraldo, M. A. Audouin, L. Massimi, C. Becares, V. Billowes, J. Cerutti, F. Cortes, G. Duran, I. Krtička, Milan Domingo-Pardo, C. Dressler, R. Carrapico, C. Berthoumieux, E. Belloni, F. Bečvář, František Bosnar, D. Barbagallo, M. Chin, M. Lederer, C. Altstadt, S. Colonna, N. Calviani, M. Cano-Ott, D. Diakaki, M. Kroll, Jiří Eleftheriadis, C. Valenta, Stanislav Dzysiuk, N. Calvino, F. Brugger, M. Chiaveri, E. Boccone, V. Andrzejewski, J.
n3:wos
000313336500005
n3:zamer
n18:MSM0021620859
s:issn
0031-9007
s:numberOfPages
5
n19:doi
10.1103/PhysRevLett.110.022501
n20:organizacniJednotka
11320