TY - JOUR
T1 - Oxalic Acid Adsorption on Rutile
T2 - Molecular Dynamics and ab Initio Calculations
AU - Biriukov, Denys
AU - Kroutil, Ondřej
AU - Kabeláč, Martin
AU - Ridley, Moira K.
AU - MacHesky, Michael L.
AU - Předota, Milan
N1 - Funding Information:
D.B., O.K., M.K., and M.P. acknowledge support from the Ministry of Education, Youth, and Sports of the Czech Republic (project LTAUSA17163). Computational resources were provided by the CESNET LM2015042 and the CERIT Scientific Cloud LM2015085, provided under the program “Projects of Large Research, Development, and Innovations Infrastructures”. M.K.R. acknowledges support from the National Science Foundation (CHE-1308726 and EAR-0842526). M.L.M. was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Chemical Sciences, Geosciences, and Biosciences Division.
Publisher Copyright:
© 2019 American Chemical Society.
PY - 2019/6/18
Y1 - 2019/6/18
N2 - Detailed analysis of the adsorption of oxalic acid ions, that is, oxalate and hydrogenoxalate, on the rutile (110) surface was carried out using molecular dynamics augmented by free energy calculations and supported by ab initio calculations. The predicted adsorption on perfect nonhydroxylated and hydroxylated surfaces with surface charge density from neutral to +0.208 C/m2 corresponding to pH values of about 6 and 3.7, respectively, agrees with experimental adsorption data and charge-distribution multisite ion complexation model predictions obtained using the most favorable surface complexes identified in our simulations. We found that outer-sphere complexes are the most favorable, owing to strong hydrogen binding of oxalic acid ions with surface hydroxyls and physisorbed water. The monodentate complex, the most stable among inner-sphere complexes, was about 15 kJ/mol higher in energy, but separated by a large energy barrier. Other inner-sphere complexes, including some previously suggested in the literature as likely adsorption structures such as bidentate and chelate complexes, were found to be unstable both by classical and by ab initio modeling. Both the surfaces and (hydrogen)oxalate ions were modeled using charges scaled to 75% of the nominal values in accord with the electronic continuum theory and our earlier parameterization of (hydrogen)oxalate ions, which showed that nominal charges exaggerate ion-water interactions.
AB - Detailed analysis of the adsorption of oxalic acid ions, that is, oxalate and hydrogenoxalate, on the rutile (110) surface was carried out using molecular dynamics augmented by free energy calculations and supported by ab initio calculations. The predicted adsorption on perfect nonhydroxylated and hydroxylated surfaces with surface charge density from neutral to +0.208 C/m2 corresponding to pH values of about 6 and 3.7, respectively, agrees with experimental adsorption data and charge-distribution multisite ion complexation model predictions obtained using the most favorable surface complexes identified in our simulations. We found that outer-sphere complexes are the most favorable, owing to strong hydrogen binding of oxalic acid ions with surface hydroxyls and physisorbed water. The monodentate complex, the most stable among inner-sphere complexes, was about 15 kJ/mol higher in energy, but separated by a large energy barrier. Other inner-sphere complexes, including some previously suggested in the literature as likely adsorption structures such as bidentate and chelate complexes, were found to be unstable both by classical and by ab initio modeling. Both the surfaces and (hydrogen)oxalate ions were modeled using charges scaled to 75% of the nominal values in accord with the electronic continuum theory and our earlier parameterization of (hydrogen)oxalate ions, which showed that nominal charges exaggerate ion-water interactions.
UR - http://www.scopus.com/inward/record.url?scp=85067473454&partnerID=8YFLogxK
U2 - 10.1021/acs.langmuir.8b03984
DO - 10.1021/acs.langmuir.8b03984
M3 - Article
C2 - 31117719
AN - SCOPUS:85067473454
SN - 0743-7463
VL - 35
SP - 7617
EP - 7630
JO - Langmuir
JF - Langmuir
IS - 24
ER -