Research Article

The Effect of Tensor Interaction in Splitting the Energy Levels of Relativistic Systems

Table 1

Energies of the spin symmetry limit in the presence and absence of Coulomb-like tensor interaction by parameters  fm−1, , ,  fm−1, = 0.4 fm−1, = 0.3 fm−1, = 0.1 fm−1, = 0.2 fm−1, and = 5 fm−1.

State () () ()State () () ()

11p1/23.8548305415.2309325021p3/23.8548305412.022333483
21d3/25.8169387916.6833417581d5/25.8169387914.646742373
31f5/27.0548784627.6122260071f7/27.0548784626.315225843
41g7/27.8556264228.2276706021g9/27.8556264227.373922639
12p1/25.7709890986.6346061852p3/25.7709890984.607350329
22d3/27.0055944557.5629965032d5/27.0055944556.267433123
32f5/27.8068061498.1800217942f7/27.8068061497.324529686
42g7/28.3464700048.6059036632g9/28.3464700048.019210395