The high-Mg mafic dykes from the Singhbhum Granitoid Complex in East India have geochemical characteristics [e.g., enrichment of the large ion lithophile elements and light rare earth elements (LREEs) relative to high field strength elements (HFSEs): high-MgO ([8 %), high-SiO 2 (C52 %), low-TiO 2 (B0.5 %), and high CaO/Al 2 O 3 (C0.58)] similar to those found in boninitic/noritic rocks. Their high percentage of orthopyroxene as a mafic mineral and of plagioclase as a felsic mineral, and normative hypersthene content greater than diopside content are also indications of their boninitic/noritic affinity. On a triangular diagram of MgO-CaO-Al 2 O 3 and on binary diagrams of Ti/V vs Ti/Sc and TiO 2 vs Zr, these samples show geochemical similarities with Phanerozoic boninites and Paleoproterozoic high-Mg norites. On major and trace element variation diagrams, these dykes show a normal crystallization trend and their Nb/La (\0.5) and Nb/Ce (\0.21) values lower than average bulk crust (0.69 and 0.33, respectively) suggest no crustal contamination. Their low values of Rb/Sr (0.11-0.41) and Rb/Ba (0.10-0.27) also suggest little or no effect of post magmatic processes. Their TiO 2 (0.27-0.50), Al 2 O 3 /TiO 2 (19.30-42.48), CaO/TiO 2 (12.96-32.52), and Ti/V (12-18) values indicate derivation from a depleted mantle source under oxidizing conditions such as a mantle wedge. Ni vs Zr modeling shows that the studied high-Mg dykes were generated by 25-30 % melting of a refractory mantle source. Enrichment of Rb, Th, U, Pb, Sr, and LREEs, and depletion of HFSEs-especially Nb, P, Ti, Zr-on primitive mantleand chondrite-normalized spider diagrams, respectively, are clear signals that the slab-derived component played an important role in the formation of melts for these rocks in a supra-subduction zone setting.