Phys.Rev. C51, 1540 (1995)

K.A.Toukan, K.Debus, F.Kappeler, G.Reffo

Stellar Neutron Capture Cross Sections of Nd, Pm, and Sm Isotopes

NUCLEAR REACTIONS ^146,148,150Nd(n, γ), E=25, 30 keV; measured Eγ, Iγ; deduced stellar capture σ(E), s-, r-, p-process abundances from ¹⁴²Nd-¹⁵⁰Sm. ¹⁴⁷Nd, ^147,148,149Pm, ^{147,148,149,150,151}Sm(n, γ), E=1-600 keV; ^146,147,148Nd, ^147,148,149Pm, ¹⁵¹Sm(n, γ), E=12-52 keV; calculated σ(E). ¹⁴⁸Nd, ^{147,148,149,150}Pm, ^{147,148,149,150,151,152,153}Sm deduced level density parameters, Γγ.

doi: 10.1103/PhysRevC.51.1540