Abstract
Density functional theory (DFT) has provided deep atomic-level insights into the adsorption behavior of aromatic molecules on solid surfaces. However, modeling the surface phenomena of large molecules on mineral surfaces with accurate plane wave methods (PW) can be orders of magnitude more computationally expensive than localized atomic orbitals (LCAO) methods. In the present work, we propose a less costly approach based on the DFT-D4 method (PBE-D4), using LCAO, to study the interactions of aromatic molecules with the {010} forsterite (Mg2SiO4) surface for their relevance in astrochemistry. We studied the interaction of benzene with the pristine {010} forsterite surface and with transition-metal cations (Fe2+ and Ni2+) using PBE-D4 and a vdW-inclusive density functional (Dion, Rydberg, Schröder, Langreth, and Lundqvist (DRSLL)) with LCAO methods. PBE-D4 shows good agreement with coupled-cluster methods (CCSD(T)) for the binding energy trend of cation complexes and with PW methods for the binding energy of benzene on the forsterite surface with a difference of about 0.03 eV. The basis set superposition error (BSSE) correction is shown to be essential to ensure a correct estimation of the binding energies even when large basis sets are employed for single-point calculations of the optimized structures with smaller basis sets. We also studied the interaction of naphthalene and benzocoronene on pristine and transition-metal-doped {010} forsterite surfaces as a test case for PBE-D4. Yielding results that are in good agreement with the plane wave methods with a difference of about 0.02-0.17 eV, the PBE-D4 method is demonstrated to be effective in unraveling the binding structures and the energetic trends of aromatic molecules on pristine and transition-metal-doped forsterite mineral surfaces. Furthermore, PBE-D4 results are in good agreement with its predecessor PBE-D3(BJM) and with the vdW-inclusive density functionals, as long as transition metals are not involved. Hence, PBE-D4/CP-DZP has been proven to be a robust theory level to study the interaction of aromatic molecules on mineral surfaces.
Original language | English |
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Pages (from-to) | 2770-2781 |
Number of pages | 12 |
Journal | Journal of Physical Chemistry A |
Volume | 125 |
Issue number | 13 |
DOIs | |
Publication status | Published - 8 Apr 2021 |
Bibliographical note
Funding Information:D.C., R.M., and A.G.G.M.T. acknowledge the E.U. under the Horizon 2020 Marie Skłodowska-Curie ITN EUROPAH (grant number 722346) and CINECA, under the ISCRA initiative, for the availability of high-performance computing resources and support. T.L. is grateful for support from NWO via a VENI fellowship (722.017.008). N.Y.D. acknowledges the UK Engineering and Physical Sciences Research Council (EPSRC) for funding (Grant No. EP/S001395/1). Studies on interstellar chemistry at Leiden Observatory are supported by a Spinoza award by the Dutch Research Council (NWO).
Funding Information:
D.C., R.M., and A.G.G.M.T. acknowledge the E.U. under the Horizon 2020 Marie Sklodowska-Curie ITN EUROPAH (grant number 722346) and CINECA, under the ISCRA initiative, for the availability of high-performance computing resources and support. T.L. is grateful for support from NWO via a VENI fellowship (722.017.008). N.Y.D. acknowledges the UK Engineering and Physical Sciences Research Council (EPSRC) for funding (Grant No. EP/S001395/1). Studies on interstellar chemistry at Leiden Observatory are supported by a Spinoza award by the Dutch Research Council (NWO).
Publisher Copyright:
© 2021 The Authors. Published by American Chemical Society.
Funding
D.C., R.M., and A.G.G.M.T. acknowledge the E.U. under the Horizon 2020 Marie Skłodowska-Curie ITN EUROPAH (grant number 722346) and CINECA, under the ISCRA initiative, for the availability of high-performance computing resources and support. T.L. is grateful for support from NWO via a VENI fellowship (722.017.008). N.Y.D. acknowledges the UK Engineering and Physical Sciences Research Council (EPSRC) for funding (Grant No. EP/S001395/1). Studies on interstellar chemistry at Leiden Observatory are supported by a Spinoza award by the Dutch Research Council (NWO). D.C., R.M., and A.G.G.M.T. acknowledge the E.U. under the Horizon 2020 Marie Sklodowska-Curie ITN EUROPAH (grant number 722346) and CINECA, under the ISCRA initiative, for the availability of high-performance computing resources and support. T.L. is grateful for support from NWO via a VENI fellowship (722.017.008). N.Y.D. acknowledges the UK Engineering and Physical Sciences Research Council (EPSRC) for funding (Grant No. EP/S001395/1). Studies on interstellar chemistry at Leiden Observatory are supported by a Spinoza award by the Dutch Research Council (NWO).