Phys.Rev. C 87, 014313 (2013)

J.Tian, N.Wang, C.Li, J.Li

Improved Kelson-Garvey mass relations for proton-rich nuclei

ATOMIC MASSES ⁵Be, ⁶B, ¹³F, ¹⁵Ne, ¹⁸Mg, ^16,17Na, ^19,20,21,22Al, ^21,22,23Si, ^{22,23,24,25,26}P, ^24,25,26,27S, ^{25,26,27,28,29,30}Cl, ^{28,29,30,31,32,33,34}K, ^{27,28,29,30,31}Ar, ^{30,31,32,33,34,35}Ca, ^{31,32,33,34,35,36,37,38}Sc, ^{33,34,35,36,37,38,39}Ti, ^{35,36,37,38,39,40,41,42,43}V, ^{37,38,39,40,41,42,43,44,45}Cr, ^{39,40,41,42,43,44,45,46,47}Mn, ^{41,42,43,44,45,46,47,48,49}Fe, ^{43,44,45,46,47,48,49,50,51,52}Co, ^{45,46,47,48,49,50,51,52,53}Ni, ^{47,48,49,50,51,52,53,54,55,56}Cu, ^{49,50,51,52,53,54,55,56,57}Zn, ⁶⁰Ga, ⁶²Ge, ⁶⁴As, ⁶⁶Se, ⁶⁸Br, ⁷⁰Kr, ⁷²Rb, ⁷⁴Sr; calculated binding energies, mass excess, S_p, S_2p using improved Kelson-Garvey (ImKG) mass relations. Comparison with experimental data for mirror analogs. Predictions of masses for proton-rich nuclides. Discussed diproton emission.

doi: 10.1103/PhysRevC.87.014313