Experimental and theoretical investigations of mercury adsorption on hematite (1-102) surfaces

Fly ash is a primary byproduct of the coal combustion process. The release of fly ash into the environment and its use in consumer products are public health concerns because of the presence of toxic trace metals and metalloids, such as mercury (Hg), selenium (Se), and arsenic (As), which may exist as components of fly ash, partition onto fly ash as it cools, or is lost to the environment through smoke stacks in a vapor phase. Therefore, it is important to understand the components of fly ash and their interaction with trace metals. In this study, calculations using density functional theory (DFT) were carried out in conjunction with experimental studies to investigate the interaction between Hg and hematite, an important mineral component of fly ash. Our experimental study, designed to simulate Hg sorption in a coal-fired power plant exhaust system, involved exposure of the fine fraction of bituminous coal fly ash (≤ 0.1 μm) to methane combustion flue gas, supplemented with SO2, NOx, HCl, and Hg in a packed-bed reactor. Sorption reaction products were characterized by synchrotron-based x-ray fluorescence mapping (s-XRF), x-ray diffraction (XRD), and extended x-ray absorption fine structure (EXAFS) spectroscopy. Preliminary s-XRF results showed that Hg in the sample is correlated with Fe, S, Cl, Br, and to a lesser extent with Se and As. From the XRD analysis, the dominant mineral phases detected were quartz, iron oxide (hematite), and various sulfate-bearing cements. Based on the experimental results, DFT studies were carried out to investigate the adsorption of Hg on hematite (α-Fe2O3) (1-102) surfaces. The two α-Fe2O3 (1-102) surfaces modeled consisted of two different surface terminations: (1) M2-clean, which corresponds to the oxygen terminated r-cut surface with the first layer of cations removed and no hydroxyl group and (2) M2-OH2-OH which has bihydroxylated top oxygen atoms and a second layer of hydroxylated oxygen atoms. These surface terminations were selected because both surfaces are highly stable in the temperature range of flue gases. All calculations were conducted using the Vienna ab-initio simulation package (VASP). Probable adsorption sites of Hg on the two α-Fe2O3 surface terminations are suggested based on calculated adsorption energies. Additionally, Bader charge analysis was conducted to characterize the oxidation state of both Hg and Fe in the α-Fe2O3 surfaces. The layer spacing of the structure was also calculated in order to compare the surface geometry before and after Hg adsorption. Preliminary results indicate that the binding energy of Hg on the M2-clean surface is -0.102 eV and that mercury donates electrons to the O and Fe atoms in the top layer when it adsorbs onto the surface.