“…Following the pioneering works carried out in the seventies (e.g., England & Richardson, 1977; Oxburgh & Turcotte, 1970, 1971; Toksöz & Bird, 1977) several key advances have been made in numerical modeling methods that have improved the understanding of the thermo‐mechanical evolution of the oceanic and continental lithosphere during oceanic subduction and continental collision (e.g., Billen, 2008; Cloos, 1982, 1983, 1993; Cloos & Shreve, 1988a, 1988b; England & Thompson, 1984; Gerya & Stöckhert, 2006; Gerya et al., 2002; Luoni et al., 2020; Magni et al., 2014; Marotta & Spalla, 2007; Peacock, 1989, 1990b; Roda et al., 2011, 2012; Thompson, 1981; van Hunen & Allen, 2011). In particular, several models have shown the importance of dehydration‐hydration reactions (e.g., Arcay et al., 2005; Faccenda et al., 2009; Faccenda & Mancktelow, 2010; Guillot et al., 2001; Meda et al., 2010; Peacock, 1990a; Quinquis & Buiter, 2014; Rupke et al., 2004; Wang et al., 2019) on the mantle wedge dynamics, with the activation of short wavelength convective cells consequent to the serpentinization and the associated decrease in viscosity (Gerya et al., 2002; Hebert et al., 2009; Hirth & Kohlstedt, 2003; Honda & Saito, 2003; Meda et al., 2010; Regorda et al., 2017; Roda et al., 2010).…”