“…The issue of vacuum stability in presence of additional scalars has been extensively studied in the literature. An incomplete list of models include SM-singlet scalar models [19][20][21][22][23][24][25], Two-Higgs doublet models (2HDM) [26][27][28][29][30][31], type-II seesaw models with SU(2) L -triplet scalars [32][33][34][35][36][37][38], U(1) extensions [39][40][41][42][43][44][45], left-right symmetric models [46][47][48], universal seesaw models [49,50], Zee-Babu model [51,52], models with Majorons [53,54], axions [22,55], moduli [56,57], scalar leptoquarks [58] or higher color-multiplet scalars [59,60], as well as various supersymmetric models [61][62][63][64]…”