“…The cognate origin model for crystallization of the MMEs from a coeval magma that gave rise to the host granitoids accounts for similar mineral assemblage and similarities in chemical and isotopic compo- sitions between enclaves and their hosts (e.g., Borodina, 1977, 1991;Dodge and Kistler, 1990;Pin et al, 1990;Dorais et al, 1997;Dahlquist, 2002;Donaire et al, 2005;Ilbeyli and Pearce, 2005;Chen et al, 2007;Shellnutt et al, 2010;Esna-Ashari et al, 2011;Flood and Shaw, 2014). In hybridism or magma mixing and/or mingling model for origin of the MMEs within the granitic pluton, the mineral, chemical, and isotopic similarities between enclaves and their hosts are commonly interpreted in terms of complete thermal and chemical equilibration between coeval, compositionally contrasted magmas in a slowly cooling plutonic body (e.g., Holden et al, 1991;Barbarin and Didier, 1992;van der Laan and Wyllie, 1993;Barbarin, 2005;Kaygusuz and Aydınçakır, 2009;Xiong et al, 2012;Zi et al, 2012;Dan et al, 2015;Ghaffari and Rashidnejad-Omran, 2015). However, others interpreted these similarities as evidence for cognate origin of the MMEs from a coeval magma that gave rise to the host granitoids (e.g., Borodina, 1977, 1991;Dodge and Kistler, 1990;Pin et al, 1990;Dorais et al, 1997;Dahlquist, 2002;Donaire et al, 2005;Ilbeyli and Pearce, 2005;Chen et al, 2007;Shellnutt et al, 2010;Esna-Ashari et al, 2011;Niu et al, 2013;Flood and Shaw, 2014;Huang et al, 2014;…”