Search of materials with C-N composition hold a great promise in creating materials which would rival diamond in hardness due to the very strong and relatively low-ionic C-N bond. Early experimental and theoretical works on C-N compounds were based on structural similarity with binary A 3 B 4 structuraltypes; however, the synthesis of C 3 N 4 remains elusive. Here we explored an unbiased synthesis from the elemental materials at high pressures and temperatures. Using in situ synchrotron X-ray diffraction and Raman spectroscopy we demonstrate synthesis of highly incompressible Pnnm CN compound with sp 3 hybridized carbon is synthesized above 55 GPa and 7000 K. This result is supported by first principles evolutionary search, which finds that Pnnm CN is the most stable compound above 10.9 GPa. On pressure release below 6 GPa the synthesized CN compound amorphizes reattaining its 1:1 stoichiometry as confirmed by Energy-Dispersive X-ray Spectroscopy. This work underscores the importance of understanding of novel high-pressure chemistry rules and it opens a new route for synthesis of superhard materials.Since the pioneering work of Liu and Cohen [1] introducing a new class of highly incompressible material, search for C 3 N 4 material harder than has diamond become the Holy Grail in the field of superhard materials. The original proposal was based on realization that carbon atoms in a hypothetical C 3 N 4 compound in the β-Si 3 N 4 structure are bound to 4 nitrogen atoms by very strong C-N bonds, which are shorter in comparison to the C-C bond in diamond (1.47 vs 1.53Å at ambient pressure) and the material is of low ionicity. In the subsequent work of Teter and Hemley [2], a number of structures with similar bonding properties have been proposed. These structures, with the exception of the graphite-like g-C 3 N 4 , have the sp 3 and sp 2 bonding for C and N atoms, respectively with the formation of CN 4 corner sharing tetrahedra (see Fig. 1(c)) where C atoms are connected with 4 N atoms and N atoms with 3 C atoms. The bulk moduli of these compounds have been calculated (using a DFT method) to be very high, exceeding that of diamond for the majority of structures, and, moreover, revealing very high densities and the presence of wide optical bandgaps (> 3 eV). These early predictions were based on the structural similarity with the known A 3 B 4 structural types, but for materials with atomic substitutions, e.g. α-and β-C 3 N 4 [2] are analogues to α-and β-Si 3 N 4 , respectively; also cubic C 3 N 4 is analogous to Th 3 P 4 .