Abstract

Head-space analysis by gas-phase infrared spectroscopy (HAGIS) allows the facile examination of the decomposition mechanisms of the metal xanthates [metal-( O-alkyldithiocarbonates], Fe(EtOCS 2) 3, Zn(EtOCS 2) 2, Cu(EtOCS 2), Pb(EtOCS 2) 2 and Ni(EtOCS 2) 2, over the temperature range 25–120°C. These metal xanthates fall into two groups based on the generation of the primary gaseous decomposition products, CS 2, COS and CO 2. The first group, consisting of Fe(III) and Zn(II) xanthates, decompose readily, forming mostly CS 2 and COS in a constant ratio and leaving, initially, a metal-alkoxide residue. In the second group, decomposition is relatively small, generating CO 2 and COS, with the proportion of COS increasing as the temperature increases and CS 2 formation occurring only at the upper end of the temperature range. The residue is more of a metal-thioalkyl species in this case. Presumably, CO 2 is formed by re-insertion of COS into a metal alkoxide and elimination of CO 2, leaving a thioalkyl moiety. Volatile metal-xanthates are probably observed in the gas-phase, allowing examination of the changes concomitant to the vaporization of the discrete metal xanthates from network or partially associated solids.

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