Phys.Rev. C 100, 054315 (2019)

Y.Y.Zong, M.Q.Lin, M.Bao, Y.M.Zhao, A.Arima

Mass relations of corresponding mirror nuclei

ATOMIC MASSES ²¹Na, ^22,23Mg, ^23,24,25Al, ^24,25,26,27Si, ^26,27,28,29P, ^28,29,30,31S, ^30,31,32,33Cl, ^32,33,34,35Ar, ^34,35,36,37K, ^36,37,38,39Ca, ^38,39,40,41Sc, ^40,41,42,43Ti, ^42,43,44,45V, ^44,45,46,47Cr, ^46,47,48,49Mn, ^48,49,50,51Fe, ^50,51,52,53Co, ^52,53,54,55Ni, ^54,55,56,57Cu, ^56,57,58,59Zn, ^58,59,60,61Ga, ^60,61,62,63Ge, ^62,63,64,65As, ^64,65,66,67Se, ^66,67,68,69Br, ^68,69,70,71Kr, ^70,71,72,73Rb, ^72,73,74,75Sr, ^74,75,76,77Y, ^76,77,78,79Zr, ^79,80Nb, ^81,83Mo, ^83,85Tc, ^85,86,87Ru, ^87,88Rh, ⁸⁹Pd; calculated mass excesses, S(n), S(p) using mass relations for corresponding mirror nuclei, and compared with AME2016 values; deduced regularities related to neutron-proton interactions, and to separation energies for mirror nuclei.

doi: 10.1103/PhysRevC.100.054315