Accurate estimates of the binding energy of nuclei far from stability that
cannot be produced in the laboratory are crucial to our understanding of
nuclear processes in astrophysical scenarios. Models based on energy density
functionals have shown that they are capable of reproducing all known masses
with root-mean-square error better than 800 keV, while retaining a firm
microscopic foundation. However, it was recently pointed out in [M. Hukkanen et
al., arXiv:2210.10674] that the recent BSkG1 model fails to account for a
contribution to the binding energy that is specific to odd-odd nuclei, and
which can be studied by using appropriate mass difference formulas. We analyse
here the (lacking) performance of three recent microscopic mass models with
respect to such formulas and examine possibilities to remedy this deficiency in
the future.Comment: 6 pages, 2 figures; Contribution to the proceedings of INPC 2022,
Cape Town, South Afric