“…We can solve the RMF equations either in the coordinate r space or in a complete basis. These equations and various extensions were already solved in r space for spherical nuclei, including the RMF equations [167,168], the relativistic Hartree-Bogoliubov (RHB) equations [169][170][171][172][173][174], the relativistic Hartree-Fock (RHF) equations [175][176][177][178][179][180], and the random phase approximation based on the RMF and RHF models [181][182][183]. For deformed nuclei, however, it is very difficult to do so because, in addition to conventional complications related to two-dimensional or three-dimensional spatial lattice techniques [184][185][186][187], one also has to deal with problems of the variational collapse 5 and fermion doubling in the relativistic framework.…”