“…In many microscopic calculations [23,24,25,26,27,28], this decrease is so large that the maximum mass obtained is not compatible with the current largest measured neutron star masses of ∼ 2M ⊙ [29,30,31,32]. Most of these microscopic calculations have been performed using NN, NNN and NY interactions and, in some cases, also the YY one [23,28]. Just a few full consistent calculations including YTBF are present in literature.…”