References quoted in the XUNDL dataset: 21NE 20NE(N,N),(N,G):RES:XUNDL-7
3 references found.
Clicking on a keynumber will list datasets that reference the given article.
Astrophys.J. 329, 943 (1988)
R.R.Winters, R.L.Macklin
Resonance Neutron Capture by 20,22Ne in Stellar Environments
NUCLEAR REACTIONS 20,22Ne(n, γ), E=2.5-200 keV; measured resonance capture yield vs E; deduced effective σ(E), Maxwellian averaged σ. 21,23Ne deduced resonances, Γγ, (gΓn).
doi: 10.1086/166438
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 90, 045804 (2014); Erratum Phys.Rev. C 92, 019902 (2015)
M.Heil, R.Plag, E.Uberseder, R.Gallino, S.Bisterzo, A.Juseviciute, F.Kappeler, C.Lederer, A.Mengoni, M.Pignatari
Stellar neutron capture cross sections of 20, 21, 22Ne
NUCLEAR REACTIONS 20,21,22Ne(n, γ), E=5-800 keV; measured transmission data, σ(E) via prompt γ-ray cascades, and using the TOF technique at the Karlsruhe Van de Graaff accelerator. 21,22,23Ne; deduced energies of neutron resonances, resonance parameters, widths, capture kernels, stellar cross sections (MACS) at kT=30 keV, relative s-abundance distributions. R-matrix analysis using SAMMY code. Comparison with previous experimental results and data in KADONIS database. Discussed 22Ne and 20Ne as significant neutron poisons for the s process in stars.
doi: 10.1103/PhysRevC.90.045804