Notes. The meaning of the parameters is as follows: N₁ and N₂ – number of 1P and 2P objects, respectively; W_o1 and W_o2 – King model parameters for 1P and 2P, respectively; Q₁ and Q₂ – virial parameters; R_g – the size of the GC circular orbit; R_h1 – half-mass radius of 1P; tidal field – tidally filling (TF) or underfilling (nTF); IMF – initial mass function; binary fraction – the ratio between the number of binaries and total objects; t_tidal− time when GC orbit size increases; conc_pop – the ratio of half-mass radii (R_h2/R_h1); m_1max and m_2max – maximum stellar masses; t_start – initial time of gas re-accretion; t_end – completion time of accretion; M_start and M_end – mass of pristine and accreted gas, respectively. The GC masses presented in this work range from 4.75 × 10⁵ M_⊙ to 3.83 × 10⁶ M_⊙ The GC models presented in this work are designed to investigate how environmental factors influence the formation and evolution of MSPs. While they are not calibrated to reproduce the full diversity of MWGCs, we use them in Section 4 to draw insights into the role of the galactic environment in shaping GC evolution.