“…• preferential exhumation of mafic high-pressure rocks from warm subduction settings that promote greater fluid productivity, mobility, and buoyancy (van Keken et al, 2018); • non-stationary (i.e., warmer, transient) temperature field in relatively young subduction zones during exhumation of some HP rocks (e.g., Willner et al, 2004;Federico et al, 2007;Krebs et al, 2008;Blanco-Quintero et al, 2011; Peacock, 2020 and references therein); • upward advection of heat by circulation of rocks in the accretionary prism and the subduction channel (Gerya et al, 2002;Gerya and Stöckert, 2006;Menant et al, 2019Menant et al, , 2020Peacock, 2020); • upward heat advection by updip percolation of slab-derived fluids within the forearc (e.g., Wang et al, 2019b); and • neglecting of additional heat sources, such as shear heating (e.g., Wada and Wang, 2009;van Keken et al, 2018;Kohn et al, 2018;Abers et al, 2020) and/or latent heating from metamorphic reactions (especially from mantle serpentinization in the upper plate, Gerya et al, 2002;Gerya and Stöckert, 2006;Kerswell et al, 2021) by simplified subduction models. Whereas some of these reasons (e.g., shear heating, Wada and Wang, 2009;Kohn et al, 2018;van Keken et al, 2018;Abers et al, 2020) have already been extensively investigated, others need systematic consideration in future numerical modeling studies.…”