Bryan Goldsmith,1 Evan Sanderson,2 Runhai Ouyang,3 Wei
Transcription
Bryan Goldsmith,1 Evan Sanderson,2 Runhai Ouyang,3 Wei
CO and NO-induced disintegration of Rh, Pd, and Pt nanoparticles on TiO2(110): A first principles study Bryan 1 Goldsmith, Evan 2 Sanderson, Runhai 3 Ouyang, Wei-Xue 3 Li 1. Department of Chemical Engineering, University of California, Santa Barbara, CA, 93106-5080 2. Department of Chemistry & Biochemistry, University of California, Santa Barbara, CA 93106-9510 3. State Key Laboratory of Catalysis, Dalian Institute of Chemical Physics, Chinese Academy of Sciences, Dalian 116023, China Free energy of reactantinduced NP disintegration Density functional theory allows the rapid calculation of the effects of reactant partial pressure (p), temperature (T), NP radius (R), as well as particle morphology on the stability of supported NPs toward disintegration into adatom complexes. Nanoparticle disintegration can cause catalyst deactivation If ΔGdisintegration is negative, then the NP should be expected to disintegrate under equilibrium conditions. Most active size [1] NP disintegration in the presence of reactants is common e.g. Rh/TiO2, Rh/Al2O3, Pd/Fe2O3, Pt/SiO2, Ir/Al2O3, Ni/TiO2, Ru/TiO2 We address the following questions: Between supported Rh, Pd and Pt catalysts, which one is more susceptible to the disintegration. Among NO and CO, which one is more efficient for the redispersion of the low surface area catalyst. How sensitive do these results depend on the particle size, temperature and partial pressure. 0 3Ωγ me px Ef ∆Gdisintegration ( R, T , p ) =− − n µ x (T , p0 ) + k BTLn − TS R p0 Nanoparticle energy Standard gas phase chemical potential An exothermic adatom complex formation energy and a small particle radius will promote NP disintegration. Increasing the reactant species chemical potential, by raising pressure or lowering temperature, will also enhance disintegration. Adatom complex formation and particle energetics CO binding on (111) facet Rh Pt Pd Projector Augmented Wave method RPBE Functional + Spin polarization Plane wave kinetic energy cutoff = 400 eV Forces converged to 0.03 eV/Å via conjugate gradient (4x2) Rutile TiO2(110) Periodic model C Rh Rh(CO) Rh(NO) diameter = 20 Å Rh(CO)2 Exp. Detected Pd and Pt not predicted to form adatom complexes CO chemical potential (eV) In agreement with experimental suggestions, Rh(NO)2 predicted to form diameter = 20 Å Exp. Suggested Pd and Pt not predicted to form adatom complexes (Under typical conditions) NO chemical potential (eV) Rh NPs are more susceptible to CO and NO-induced disintegration compared to both Pd and Pt NPs, and NO is a greater promoter of NP disintegration than CO. The facile disintegration of Rh NPs is due to the large and exothermic formation energy of the Rh adatom complexes. These findings provide insights for how to either prevent or promote reactant-induced NP disintegration. contours (Ω is molar volume) R In the presence of NO ∆ E NP eV eV Rh(CO)2 -1.35 eV These trends, which are manifested by the interplay between coverage dependent adsorption energies, reactant-induced surface stabilization, and NP size, give insight into the variability of particle stability over a broad range of reaction conditions. The interaction between CO and NO with the Rh adatom is greater than for the Pd and Pt adatoms. The Rh/TiO2(110) NPs are less resistant to CO and NO-induced disintegration than the Pd/TiO2(110) and Pt/TiO2(110) NPs NO is a more efficient reactant for particle redispersion than CO Future work Include gas phase disintegration Consider adatom translation Particle size-dependent binding energies Pd(CO)2 (g) Rh(NO)2 Vacuum layer thickness of 15 Å Bottom two tri-layers are fixed in positions. Pd NO chemical potential (eV) LESS STABLE Formation energy = 0.75 eV N Rh Pt Reactant environment and particle size effects on supported nanoparticle energy ΔE NP = not detected Conclusions Most stable adatom positions on TiO2(110), corresponding to formation energies of 2.88, 2.01 and 3.12 eV for Rh, Pd, and Pt, respectively. O NO binding on (111) facet Temperature ↓, Pressure ↑, Coverage ↑ 3Ω γ(111) In agreement with experiment, Rh(CO)2 predicted to form but not Rh(CO) In the presence of NO CO chemical potential (eV) In the presence of CO E formation = Eadatom/support − Esupport − Ebulk Reduction in surface energy due to reactant binding CO and NO bind strongest to Rh metal compared to Pd and Pt metals MORE STABLE Density Functional Theory modeling using Vienna Ab-initio Simulation Package At a specified gas phase chemical potential, the adatom complex that is most likely to form has the most negative disintegration free energy. In the presence of CO 111 111 [ ( , )] f T P γ γ γ γ + ∆ ≈ + ∆ ∑i i i me me (T , P ) ∆ E NP Computational Methodology 0.09 -0.69 -0.10 -0.68 i Reduction in surface energy (eV/Å2) Configurational entropy of complexes Formation energy of adatom complex 0.26 -0.54 -0.05 -0.67 Exothermic formation energy promotes particle disintegration Influence of CO and NO adsorption on �𝒎𝒎 Pt, Pd, or Rh nanoparticle surface energetics 𝜸 (T , P) γ me = [1] 0.75 -1.35 -0.02 -1.58 Pt Gibbs free energy of disintegration (eV) ∆Gdisintegration < 0 Disintegration Pd Energies are in eV. Disintegration can be modeled by the Gibbs Free Energy Rh/SiO2 Rh Gibbs free energy of disintegration (eV) Disintegration of supported nanoparticles (NPs) in the presence of reactants can lead to catalyst deactivation or be exploited to redisperse sintered catalysts. Formation energy Metal(CO) Metal(CO)2 Metal(NO) Metal(NO)2 Reduction in surface energy (eV/Å2) Introduction Pt, Pd, Rh NP/TiO2(110) disintegration The interaction of CO and NO with Rh adatom is greater than for Pd and Pt adatoms -1.58 eV -0.02 eV Rh(CO)2 and Rh(NO)2 have more favorable formation energies than Rh(CO) and Rh(NO) Acknowledgments References This work was funded by the NSFC (21173210, 21225315), the 973 Program (2013CB834603), and the NSF-OISE 0530268. B.R.G. acknowledges the PIRE-ECCI program for a graduate fellowship. E.D.S. thanks IRES-ECCI for an undergraduate summer research fellowship. [1] McClure, S. M.; Lundwall, M. J.; Goodman, D. W. Proc. Natl. Acad. Sci. 2011, 108, 931 [2] Ouyang, R.; Liu, J.-X.; Li, W.-X. J. Am. Chem. Soc. 2012, 135, 1760