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2019YU03      Phys.Rev. C 100, 014314 (2019)

H.C.Yu, M.Q.Lin, M.Bao, Y.M.Zhao, A.Arima

Empirical formulas for nuclear separation energies

NUCLEAR STRUCTURE ^{70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100}Zn, ^{112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137}Mo, ^{151,152,153,154,155,156,157,158,159,160,161,162,163,164,165,166,167,168,169,170,171,172,173,174,175,176,177,178,179,180,181,182,183,184,185,186}Ba, ^{204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239}W; calculated S(n) and S(p) using empirical formulas. Comparison with AME-2016 evaluation, and with other theoretical model predictions.

doi: 10.1103/PhysRevC.100.014314
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