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1993RA24      Astrophys.J. 419, 207 (1993)

C.M.Raiteri, R.Gallino, M.Busso, D.Neuberger, F.Kappeler

The Weak s-Component and Nucleosynthesis in Massive Stars

NUCLEAR REACTIONS ⁸⁷Rb(n, γ), E=25, 30 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties.

COMPILATION ^58,59,60Fe, ^59,60Co, ^{58,59,60,61,62,63,64}Ni, ^63,64,65Cu, ^{64,65,66,67,68,70}Zn, ^69,71Ga, ^{70,71,72,73,74,76}Ge, ⁷⁵As, ^{76,77,78,79,80,82}Se, ^79,80,81Br, ^{80,81,82,83,84,85,86}Kr, ^85,86,87Rb, ^{86,87,88,89,90}Sr, ^89,90Y, ^{90,91,92,93,94,96}Zr(n, γ), E=26, 91 keV; compiled experimental and theoretical (n, γ) Maxwellian-averaged σ and their uncertainties.

doi: 10.1086/173476
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