References quoted in the XUNDL dataset: 63NI 62NI(N,G):RESONANCES:XUNDL-4
3 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Rev. 159, 1007 (1967)
R.L.Macklin, J.H.Gibbons
Capture-Cross-Section Studies for 30-220-keV Neutrons Using a New Technique
NUCLEAR REACTIONS V, Fe, Ni, 86,87Sr, Y, Nb, Rh, Ag, 122,123,124,125,126,128,130Te, I, Eu, 175,176Lu, W, Au, 204,208Pb(n, γ), E=30-220 keV; measured reaction products, Eγ, Iγ; deduced σ and their uncertainties.
Chin.Phys.C 36, 1603 (2012)
M.Wang, G.Audi, A.H.Wapstra, F.G.Kondev, M.MacCormick, X.Xu, B.Pfeiffer
The AME2012 atomic mass evaluation (II). Tables, graphs and references
COMPILATION A=1-295; compiled, evaluated atomic mass data.
Phys.Rev. C 89, 025810 (2014); Erratum Phys.Rev. C 92, 019903 (2015)
C.Lederer, for the n_TOF Collaboration
62Ni(n, γ) and 63Ni(n, γ) cross sections measured at the n_TOF facility at CERN
NUCLEAR REACTIONS 62Ni(n, γ), E<200 keV; 63Ni(n, γ), E=10-270 keV; measured Eγ, Iγ, neutron time-of-flight, capture yields, σ(E) at n_TOF-CERN facility. 63,64Ni; deduced resonance energies, levels, neutron and gamma widths, kernels, level spacing, Maxwellian averaged cross sections (MACS). Comparison with previous measurements, KADoNiS compilation, and ENDF/B-VII.1, JENDL-4.0, and JEFF-3.1.1 libraries. Discussed constraints on s-process production of heavier species and Cu in massive stars.
doi: 10.1103/PhysRevC.89.025810