Models suggest BrHgONO to be the major Hg(II) species formed in the global oxidation of Hg(0), and BrHgONO undergoes rapid photolysis to produce the thermally stable radical BrHgO • . We previously used quantum chemistry to demonstrate that BrHgO • can, like • OH radicals, readily abstract hydrogen atoms from sp 3 -hybridized carbon atoms as well as add to NO and NO 2 . In the present work, we reveal that BrHgO • can also add to C 2 H 4 to form BrHgOCH 2 CH 2 •, although this addition appears to proceed with a lower rate constant than the analogous addition of • OH to C 2 H 4 . Additionally, BrHgO • can readily react with HCHO in two different ways: either by addition to carbon or by abstraction of a hydrogen atom. The minimum energy path for the BrHgO • + HCHO reaction bifurcates, forming two prereactive complexes, each of which passes over a separate transition state to form different products. Rate constants computed using Master Equation simulations indicate that hydrogen abstraction dominates over addition at atmospheric temperatures (200 K ≤ T ≤ 333 K) and pressures (0.01 atm ≤ P ≤ 1 atm). Subsequently, we compute the atmospheric fate of BrHgO • in a variety of air masses and find that BrHgOH formation via hydrogen abstraction will be the predominant fate (∼70–99%), with major competition (∼20%) coming from addition to NO and NO 2 in polluted urban regions and stratospheric air. Given the absence of either field data on the identity of Hg(II) compounds or experimental data on the kinetics of BrHgO • reactions, the present manuscript should provide guidance to a range of scientists studying atmospheric mercury.
No takes yet. Share an insight, caveat, or question.
Lam et al. (2019) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: