Phys.Rev. C 103, 054326 (2021)

C.Ma, Y.Y.Zong, S.Q.Zhang, J.Li, K.Wang, Y.M.Zhao, A.Arima

Mass relations of mirror nuclei in terms of Coulomb energies based on relativistic continuum Hartree-Bogoliubov calculations

ATOMIC MASSES ^18,19Ne, ^19,20,21Na, ^20,21,22,23Mg, ^{21,22,23,24,25}Al, ^{22,23,24,25,26,27}Si, ^{24,25,26,27,28,29}P, ^{27,28,29,30,31}S, ^{29,30,31,32,33}Cl, ^32,33,34,35Ar, ^{33,34,35,36,37}K, ^{35,36,37,38,39}Ca, ^38,39,40,41Sc, ^40,41,42,43Ti, ^{41,42,43,44,45}V, ^{43,44,45,46,47}Cr, ^{44,45,46,47,48,49}Mn, ^{46,47,48,49,50,51}Fe, ^{49,50,51,52,53}Co, ^{50,51,52,53,54,55}Ni, ^{53,54,55,56,57}Cu, ^56,57,58,59Zn, ^59,60,61Ga, ^60,61,62,63Ge, ^62,63,64,65As, ^65,66,67Se, ^67,68,69Br, ^69,70,71Kr, ^71,72,73Rb, ^73,74,75Sr, ^75,76,77Y, ^78,79Zr, ⁸¹Nb, ⁸³Mo, ⁸⁵Tc, ⁸⁷Ru; calculated mass excesses, S(p), S(2p) of mirror nuclei, including masses of 61 unknown proton-rich nuclei, in terms of Coulomb energies based on relativistic continuum Hartree-Bogoliubov (RCHB) method. Numerical values listed in Supplemental material of the paper. Comparison with values in AME2016 database.

doi: 10.1103/PhysRevC.103.054326