Computational Study on the Photolysis of BrHgONO and the Reactions of BrHgO• with CH4, C2H6, NO, and NO2: Implications for Formation of Hg(II) Compounds in the Atmosphere

Global models suggest BrHgONO to be the major Hg(II) species initially formed in atmospheric oxidation of Hg(0) in most of the atmosphere, but its atmospheric fate has not been previously investigated. In the present work, we use quantum chemistry to predict that BrHgONO photolysis produces the thermally stable radical BrHgO • . Subsequently, BrHgO • may react with NO 2 to form thermally stable BrHgONO 2, or with NO to re-form BrHgONO. Additionally, BrHgO • abstracts hydrogen atoms from CH 4 and C 2 H 6 with higher rate constants than does • OH, producing a stable BrHgOH molecule. Because BrHgO • can abstract hydrogen atoms from sp 3 -hybridized carbons on many organic compounds, we expect production of BrHgOH to dominate globally, although formation of BrHgONO and BrHgONO 2 may compete in urban regions. In the absence of experimental data on the kinetics and fate of BrHgONO and BrHgO •, we aim to guide modelers and other scientists in their search for Hg(II) compounds in the atmosphere.