Prog.Part.Nucl.Phys. 66, 368 (2011)

H.Lenske, S.E.A.Orrigo, N.Tsoneva

Density functional theory for reactions of astrophysical interest

NUCLEAR STRUCTURE ^{100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132}Sn; calculated electric dipole strength distributions, B(E1), nuclear skin thickness. QRPA results.

NUCLEAR REACTIONS ¹³⁸Ba(γ, X), E<9 mEV; calculated photo-absorption σ. QRPA results.

doi: 10.1016/j.ppnp.2011.01.036