Chinese Journal of Chemical Physics  2017, Vol. 30 Issue (6): 685-690

The article information

Xi-zi Cao, Bao-qi Yin, Ting-ting Wang, Xiao-peng Xing
曹西子, 殷保祺, 王亭亭, 邢小鹏
Exploring the Interactions of Atomic Oxygen on Silver Clusters with Hydrogen
银团簇上吸附氧原子与氢气作用的研究
Chinese Journal of Chemical Physics, 2017, 30(6): 685-690
化学物理学报, 2017, 30(6): 685-690
http://dx.doi.org/10.1063/1674-0068/30/cjcp1710193

Article history

Received on: October 23, 2017
Accepted on: December 4, 2017
Exploring the Interactions of Atomic Oxygen on Silver Clusters with Hydrogen
Xi-zi Cao, Bao-qi Yin, Ting-ting Wang, Xiao-peng Xing     
Dated: Received on October 23, 2017; Accepted on December 4, 2017
School of Chemical Science and Engineering, Shanghai Key Laboratory of Chemical Assessment and Sustainability, Tongji University, Shanghai 200092, China
*Author to whom correspondence should be addressed. Xiao-peng Xing, E-mail:xingxp@tongji.edu.cn
Part of the special issue for "the Chinese Chemical Society's 15th National Chemical Dynamics Symposium"
Abstract: The interactions between AgnO-(n=1-8) and H2 (or D2) were explored by combination of the mass spectroscopy experiments and density function theory (DFT) calculations. The experiments found that all oxygen atoms in AgnO-(n=1-8) are inert in the interactions with H2 or D2 at the low temperature of 150 K, which is in contrast to their high reactivity with CO under the same condition. These observations are parallel with the preferential oxidation (PROX) of CO in excess hydrogen catalyzed by dispersed silver species in the condensed phase. Possible reaction paths between AgnO-(n=1-8) and H2 were explored using DFT calculations. The results indicated that adsorption of H2 on any site of AgnO-(n=1-8) is extremely weak, and oxidation of H2 by any kind of oxygen in AgnO-(n=1-8) has an apparent barrier strongly dependent on the adsorption style of the "O". These experiments and theoretical results about cluster reactions provided molecule-level insights into the activity of atomic oxygen on real silver catalysts.
Key words: Silver clusters    Atomic oxygen    Hydrogen    Mass spectroscopy    Density function theory calculations    
Ⅰ. INTRODUCTION

The reactivity of oxygen species on silver is a very import topic in the surface science, because it is closely relevant to many industrially or environmentally important oxidation processes catalyzed by silver, such as the partial oxidation of ethylene or propylene [1], and selective oxidation of CO from hydrogen-rich gas used in fuel cells [2, 3]. Extensive studies were carried out on the structures and properties of oxygen species on bulk silver or dispersed silver particles, showing that they have quite a few various molecular and atomic states [4, 5]. The atomic oxygen on silver was classified to three types, O$_\alpha$ (the weakly adsorbed oxygen atoms on surfaces), O$_\beta$ (the atomic oxygen inside bulks), and O$_\gamma$ (the strongly adsorbed atomic oxygen in crevices or embedded in sub surfaces). They generally have different performances in surface reactions, and this classification was widely used to analyze the catalytic mechanisms on silver [6-8]. With developments of modern surface techniques, more details of the atomic oxygen on silver were resolved [9, 10]. Nevertheless, because of the intrinsic complexities of the solids, there are still many challenges to locate the exact positions of various oxygen atoms on silver, to determine their bonding patterns, and to elucidate their structure-property relations at molecule level.

Silver clusters are ideal models for the active sites of heterogeneous silver catalysts, and many of them were studied using gas phase experiments and density function theory calculations [11-23]. The structures and properties of these small species have many distinctive characters. For example, some small clusters have kind of global or local five-fold symmetry [17, 18], which can not exist in crystals. The adsorption, activation and reactions of O$_2$ on Ag$_n$$^-$ were explored by many groups [24-30], and clusters' spins and electron bonding energies were shown to dominate the reactions. Our recent study showed that this tendency is still true for the clusters with sizes up to 1 nm [31]. Except the reactions with O$_2$, there were also lots of studies about the reactions of silver clusters with other molecules, like ethylene, CO, NO$_x$, etc. [32-36]. However, there were few studies involving chemical properties of adsorbed heterogeneous atoms (including the important atomic oxygen) on silver clusters, even though they are as well directly relevant to real catalytic processes.

In our recent study [37], we generated cluster series AgnO- (n=1-8), and explored their reactions with CO. In this work, we explored the interactions between AgnO- (n=1-8) and H$_2$ or D$_2$. We also studied the reactions of AgnO- with CO mixed in the D$_2$. In these experiments, H$_2$ and D$_2$ do not react with AgnO-, Ag$_n$$^-$ and other products from CO reactions. The DFT calculations predicted the adsorption energies of H$_2$ on the above clusters and the possible reaction paths between AgnO- (n=1-8) and H$_2$. The theoretical results well interpreted the experimental observations. The experiments and the theoretical calculations of these cluster species can be used to understand the processes happening on the active sites of real silver catalysts.

Ⅱ. EXPERIMENTAL AND COMPUTATIONAL METHODS A. Measurements on clusters' reactions

The measurements on clusters' reactions were carried out on an instrument composed of a magnetron sputter cluster source, a flow reactor, and a time-of-flight (TOF) mass spectrometer, whose details were described elsewhere [31, 38, 39]. Briefly, the cluster source generated the AgnO- (n=1-8) series by mixing trace amount of oxygen (at a ppm level) inside the helium buffer gas, in which the O$_2$ molecules dissociated and combined with silver species around the sputtering region. Together with the buffer gas (110 sccm helium) and the sputtering gas (14 sccm Ar), all clusters from the cluster source entered a continuous flow reactor running at 150 K. They firstly went through a thermalization area, and then entered the reaction area, where the reactant was introduced at a defined flow rate. Since the oxygen mixed inside the buffer gases was at ppm levels, its effect on the subsequent reactions in the reactor was negligible. The parent and product clusters were sampled by a skimmer at the end of the reactor and were directed to the TOF mass spectrometer to be analyzed.

B. Density functional theory (DFT) calculations

The clusters' reaction paths were investigated using DFT calculations. The B3LYP hybrid functional was used [40-42], which makes use of the Hartree-Fock exact exchange and Becke's exchange functional and the Lee-Yang-Parr correlation functional. The structural candidates of the reactants, the intermediates, the products, and the transition states were initially optimized with the Lanl2dz basis sets for all elements. The lower lying ones from these preliminary calculations were further optimized using a more sophisticated method, in which the aug-cc-pVTZ-pp basis set was selected for Ag, and the 6-311G$^*$ basis sets for C and O [43]. Scalar and spin-orbital relativistic effects of Ag were taken into account via the energy consistent relativistic pseudopotentials. The predicted structures for the minimum points and the transition states were confirmed by analyzing their vibration modes, which have no and only one imaginary frequency, respectively. Using the intrinsic reaction coordinate (IRC) algorithm, we traced the reaction paths from transition states to the corresponding reactants and products to reconfirm the proposed reaction mechanism. All calculations were accomplished using Gaussian 09 program [44].

Ⅲ. RESULTS AND DISCUSSION A. Measurements on interactions of AgnO- (n=1-8) with H$_\textbf{2}$ (D$_\textbf{2}$) or CO mixed in D$_\textbf{2}$

FIG. 1 shows the mass spectra of anionic clusters sampled at the end of the reactor with no reactants, with 0.20 sccm H$_2$, and with 0.20 sccm D$_2$, respectively. Because the mass resolution (m/$\Delta m$) of these spectra is around 500, the experiments would clearly distinguish the adsorption products of H$_2$ or D$_2$ on AgnO- (n=1-8) and Ag$_n$$^-$ (n=1-11) if they were ever generated. Nevertheless, the mass spectrum shown in FIG. 1 (b) or (c), with high flow of H$_2$ or D$_2$ introduced, is nearly identical to that of FIG. 1(a). That is to say, neither addition of H$_2$ or D$_2$ on Ag$_n$$^-$ and AgnO-, nor reduction of AgnO- to Ag$_n$$^-$ happened under the present low temperature condition. FIG. 2 shows the mass spectra of anionic clusters sampled at the end of the reactor without reactants, with pure 0.05 sccm CO, with 0.05 sccm CO mixed in 0.10 sccm D$_2$, and with 0.10 sccm CO mixed in 0.20 sccm D$_2$, respectively. Similar to FIG. 1(a), the mass spectrum in FIG. 2(a) mainly includes two cluster series, Ag$_n$$^-$ (n=1-11) and AgnO- (n=1-8). FIG. 2(b) indicates that the addition of CO leads to reduction of AgnO- (n=1, 2, 5-8) to the corresponding Ag$_n$$^-$, and the formation of Ag$_3$CO$_2$$^-$ and Ag$_4$CO$_2$$^-$ from Ag3O- and Ag4O-, respectively. These reactions were discussed in our previous work [37]. The mass spectrum in FIG. 2(c), showing the products of cluster reactions with CO mixed in D$_2$, is nearly identical to that in FIG. 2(b), for which only same amount of CO was introduced. The only difference is that the small impurity cluster peaks for AgOH$^-$ in FIG. 2(b) (actually also exists without any reactants in FIG. 1(a) and FIG. 2(a)) changed to AgOH$^-$/AgOD$^-$. This indicates that the presence of D$_2$ did not affect the reaction kinetics of AgnO- (n=1-8) with CO at all. As shown in FIG. 2(d), when the flow of the reactants CO and D$_2$ doubled in the reactor compared with that of FIG. 2(c), the reactions from AgnO- (n=1, 2, 5-8) to Ag$_n$$^-$, and from Ag3, 4O- to Ag$_{3, 4}$CO$_2$$^-$ were driven to 100% completion. The intensity of AgOD$^-$ did not increase, indicating that this cluster was not generated in the reactor. In both FIG. 2 (c) and (d), no addition products of D$_2$ were observed on Ag$_n$$^-$, AgnO-, or the formed Ag$_n$CO$_2$$^-$; no reduction reactions from AgnO- to Ag$_n$$^-$ were observed either.

FIG. 1 Mass spectra showing the cluster series of AgnO- (n=1-8) and Ag$_n$$^-$ (n=1-11) with (a) no reactant, (b) 0.20 sccm H$_2$ and (c) 0.20 sccm D$_2$ introduced into the reactor at 150 K. The peaks of Ag$_n$$^-$ (n=1-8) were indicated with vertical dashed lines; the peaks of AgnO- series were indicated using "+O".
FIG. 2 Mass spectra showing the cluster series of AgnO- (n=1-8) and Ag$_n$$^-$ (n=1-11) with (a) no reactant, (b) 0.05 sccm CO mixed in 0.10 sccm D$_2$, and (c) 0.10 sccm CO mixed in 0.20 sccm D$_2$ introduced into the reactor at 150 K. The peaks of Ag$_n$$^-$ (n=1-8) are indicated with vertical dashed lines; the peaks of AgnO- series and other clusters are indicated using the extra atom or group added to the corresponding Ag$_n$$^-$.
B. Theoretical calculations on proposed reactions between AgnO- and H$_\textbf{2}$

The lowest structures of AgnO- (n=1-8) and their reactions with CO were previously explored [37]. In this work, we explored the possible reaction paths of previous determined structures of AgnO- (n=1-8) with H$_2$ using DFT calculations, even though no reactions were observed under the present low temperature. The predicted reaction paths were listed in FIG. 3, including the structures and the relative energies of the involved reactants, the intermediates, the final products, and the transition states.

FIG. 3 Theoretical paths for the reactions between AgnO- (n=1-8) and H$_2$. The structures and the relative energies of the reactants, the intermediates, the transition states, and the products were included.

The predicted H$_2$ adsorption energies on any site of Ag$_n$$^-$ (n=1-11), AgnO- (n=1-8), and Ag$_n$CO$_2$$^-$ (n=3 and 4) are close to zero, and some of them are even slightly negative. The higher energies of the adsorption minima, i.e. the theoretical negative adsorption energies, can be caused by deviations from the intrinsic limitations of DFT methods in predicting the extremely weak nonbonding interactions. However, the results at least showed that the adsorption of H$_2$ on any of these clusters is very weak, which is consistent with the experimental observations that no H$_2$ adsorption products presented in the obtained mass spectra. When a H$_2$ molecule was put around AgnO- (n=1-8), the theoretical optimization unexceptionally converged to the structures with H$_2$ staying around the oxygen atom. The most stable product of AgnO- (n=1, 2, 5-8) and H$_2$ was predicted to be Ag$_n$$^-$ taking an adsorbed H$_2$O, in which the two hydrogen atoms were oriented toward the Ag$_n$$^-$. The relative energies of these products were more than 1.0 eV lower than those of the corresponding reactants, AgnO-+H$_2$, and 0.3-0.6 eV lower than those of separate Ag$_n$$^-$ and H$_2$O. The oxidations of H$_2$ by the oxygen in the quasi-linear structures of Ag3O- and Ag4O- were predicted to form AgH$_2$OAg$_2$$^{-}$ and AgH2OAg2-, respectively. In these two structures, each H$_2$O unit connected two silver fragments using the oxygen atom and one of its hydrogen atoms. The fragmentation of AgH$_2$OAg$_2$$^-$ and AgH2OAg2- needs at least 1.06 and 0.87 eV, respectively. Their structures and fragmentation are very similar to those of previously observed AgCO$_2$Ag$_2$$^-$ and Ag$_2$CO$_2$Ag$_2$$^-$ [37]. The relative energies of AgH$_2$OAg$_2$$^-$ and AgH2OAg2- are more than 1.0 eV lower than those of their initial reactants, Ag3O-+H$_2$ and Ag4O-+H$_2$. FIG. 3 also listed the structures and the energies of the transition states of the proposed reactions between AgnO- (n=1-8) and H$_2$. The main barriers in the reactions of AgO$^-$ and Ag2O-, which contain terminal oxygen, were estimated to be 0.19 eV; those of Ag3O- and Ag4O-, which contain Ag-O-Ag linear structures, were estimated to be 0.47 and 0.28 eV, respectively; those of AgnO- (n=5-8), which contain bridge oxygen atoms, were estimated to be 0.6-1.2 eV. These theoretical results are consistent with the experimental observations that all AgnO- (n=1-8) can not react with H$_2$ or D$_2$ at the low temperature.

C. Comparing the gas phase results with surface studies about atomic oxygen in condensed phases

The reactivity of surface oxygen on silver was extensively investigated in condensed phases. It was shown that most atomic oxygen on silver reacts with CO below 200 K [45-48], while activation or reactions of H$_2$ on these oxygen species generally happen at temperatures higher than 400 K [49-52]. This difference is the fundamental for applications of silver catalysts in selective oxidation of CO from H$_2$-rich gas in fuel cells, where the Pt anodes are easily poisoned by traces of CO. The significant barriers for the reactions with hydrogen revealed in this work and the previously reported barrierless reactions with CO provide the underlying molecule-level interpretation. We also noticed that the barriers in the reactions of AgnO- with H$_2$ are strongly dependent on the adsorption structures of atomic oxygen. The terminal oxygen corresponds to the lowest reaction barriers; those of the quasi-linear structures of Ag-O-Ag are slightly higher; those of the bridging ones, especially the ones bridging on two silver atoms, are the highest ones and can be more than 1.0 eV. This implies that those different atomic oxygen tend to activate or react with H$_2$ at different high temperatures. In condensed phases, the pretreatment of silver catalysts at high temperatures with presence of H$_2$ was shown to significantly change their activity and selectivity, and the temperature is usually among the most important parameters [2, 3, 53]. According to the micro figures revealed in this work, different pretreatment temperatures lead to removal of various atomic oxygen. The population of different kinds of atomic oxygen on silver directly determines the subsequent reaction mechanisms in the catalytic processes.

Ⅳ. CONCLUSION

We explored the reactions of AgnO- with hydrogen (H$_2$ or D$_2$), and CO mixed in D$_2$. It was found that all atomic oxygen in AgnO- (n=1-8) does not react with H$_2$ or D$_2$ at 150 K, which is in contrast to their high reactivity with CO under the same condition. The theoretical calculations predicted the barriers of the reactions between AgnO- and H$_2$, which are strongly dependent on the adsorption structures of the atomic oxygen. These results provide molecule-level understanding on the catalytic process of selective oxidation of CO from H$_2$-rich gas in fuel cells and the pretreatment process of silver catalysts with presence of H$_2$.

Ⅴ. ACKNOWLEDGMENTS

This work was supported by the National Natural Science Foundation of China (No.21273278 and No.21673158), the Ministry of Science and Technology of China (No.2012YQ22011307), and Science & Technology Commission of Shanghai Municipality (14DZ2261100). The authors are greatly thankful to Dr. Joel H. Parks in Rowland Institute at Harvard for giving us most of the experimental facilities, and acknowledge helpful discussions with Prof. Xue-feng Wang in Tongji University.

Reference
[1] R. M. Lambert, F. J. Williams, R. L. Cropley, and A. Palermo, J. Mol. Catal. A:Chem. 228 , 27 (2005). DOI:10.1016/j.molcata.2004.09.077
[2] Z. Qu, M. Cheng, C. Shi, and X. Bao, J. Mol. Catal. A:Chem. 239 , 22 (2005). DOI:10.1016/j.molcata.2005.05.033
[3] Z. Qu, M. Cheng, X. Dong, and X. Bao, Catal. Today 247 , 93–95 (2004).
[4] C. T. Campbell, Surf. Sci. 157 , 43 (1985). DOI:10.1016/0039-6028(85)90634-X
[5] F. Besenbacher, and J. K. Nørskov, Prog. Surf. Sci. 44 , 5 (1993). DOI:10.1016/0079-6816(93)90006-H
[6] A. J. Nagy, G. Mestl, and R. Schlögl, J. Catal. 188 , 58 (1999). DOI:10.1006/jcat.1999.2651
[7] S. Linic, and M. A. Barteau, J. Am. Chem. Soc. 125 , 4034 (2003). DOI:10.1021/ja029076g
[8] G. I. N. Waterhouse, G. A. Bowmaker, and J. B. Metson, Appl. Surf. Sci. 214 , 36 (2003). DOI:10.1016/S0169-4332(03)00350-7
[9] D. S. Su, T. Jacob, T. W. Hansen, D. Wang, R. Schloegl, B. Freitag, and S. Kujawa, Angew. Chem. Int. Edit. 47 , 5005 (2008). DOI:10.1002/anie.v47:27
[10] T. C. R. Rocha, A. Oestereich, D. V. Demidov, M. Haevecker, S. Zafeiratos, G. Weinberg, V. I. Bukhtiyarov, A. Knop-Gericke, and R. Schloegl, Phys. Chem. Chem. Phys. 14 , 4554 (2012). DOI:10.1039/c2cp22472k
[11] H. Handschuh, C. Y. Cha, P. S. Bechthold, G. Ganteför, and W. Eberhardt, J. Chem. Phys. 102 , 6406 (1995). DOI:10.1063/1.469356
[12] S. Kruckeberg, G. Dietrich, K. Lutzenkirchen, L. Schweikhard, C. Walther, and J. Ziegler, Int. J. Mass Spectrom. Ion Processes 155 , 141 (1996). DOI:10.1016/S0168-1176(96)04412-6
[13] K. Michaelian, N. Rendon, and I. L. Garzon, Phys. Rev. B 60 , 2000 (1999). DOI:10.1103/PhysRevB.60.2000
[14] I. Rabin, W. Schulze, and G. Ertl, Chem. Phys. Lett. 312 , 394 (1999). DOI:10.1016/S0009-2614(99)00872-6
[15] V. A. Spasov, T. H. Lee, J. P. Maberry, and K. M. Ervin, J. Chem. Phys. 110 , 5208 (1999). DOI:10.1063/1.478416
[16] P. Weis, T. Bierweiler, S. Gilb, and M. M. Kappes, Chem. Phys. Lett. 355 , 355 (2002). DOI:10.1016/S0009-2614(02)00277-4
[17] X. P. Xing, R. M. Danell, I. L. Garzon, K. Michaelian, M. N. Blom, M. M. Burns, and J. H. Parks, Phys. Rev. B 72 , 081405 (2005). DOI:10.1103/PhysRevB.72.081405
[18] D. Schooss, M. N. Blom, J. H. Parks, B. von Issendorff, H. Haberland, and M. M. Kappes, Nano Lett. 5 , 1972 (2005). DOI:10.1021/nl0513434
[19] M. N. Blom, D. Schooss, J. Stairs, and M. M. Kappes, J. Chem. Phys. 124 , 244308 (2006). DOI:10.1063/1.2208610
[20] X. L. Yang, W. S. Cai, and X. G. Shao, J. Phys. Chem. A 111 , 5048 (2007). DOI:10.1021/jp0711895
[21] M. Harb, F. Rabilloud, D. Simon, A. Rydlo, S. Lecoultre, F. Conus, V. Rodrigues, and C. Felix, J. Chem. Phys. 129 , 194108 (2008). DOI:10.1063/1.3013557
[22] S. Y. Yan, W. Zhang, Z. X. Zhao, W. C. Lu, and H. X. Zhang, Theor. Chem. Acc. 131 , 1200 (2012). DOI:10.1007/s00214-012-1200-4
[23] G. U. Gamboa, A. C. Reber, and S. N. Khanna, New J. Chem. 37 , 3928 (2013). DOI:10.1039/c3nj01075a
[24] L. D. Socaciu, J. Hagen, U. Heiz, T. M. Bernhardt, T. Leisner, and L. Woste, Chem. Phys. Lett. 340 , 282 (2001). DOI:10.1016/S0009-2614(01)00447-X
[25] M. Schmidt, A. Masson, and C. Bréchignac, Phys. Rev. Lett. 91 , 243401 (2003). DOI:10.1103/PhysRevLett.91.243401
[26] L. D. Socaciu, J. Hagen, J. Le Roux, D. Popolan, T. M. Bernhardt, L. Woste, and S. Vajda, J. Chem. Phys. 120 , 2078 (2004). DOI:10.1063/1.1644103
[27] J. Hagen, L. D. Socaciu, J. Le Roux, D. Popolan, T.M. Bernhardt, L. Woste, R. Mitric, H. Noack, and V. Bonacic-Koutecky, J. Am. Chem. Soc. 126 , 3442 (2004). DOI:10.1021/ja038948r
[28] Z. Luo, G. U. Gamboa, J. C. Smith, A. C. Reber, J. U. Reveles, S. N. Khanna, and A. W. Castleman Jr., J. Am. Chem. Soc. 134 , 18973 (2012). DOI:10.1021/ja303268w
[29] Y. N. Wu, M. Schmidt, J. Leygnier, H. P. Cheng, A. Masson, and C. Brechignac, J. Chem. Phys. 136 , 8 (2012).
[30] M. Schmidt, A. Masson, H. P. Cheng, and C. Brechignac, Chemphyschem 16 , 855 (2015). DOI:10.1002/cphc.v16.4
[31] J. Ma, X. Cao, X. Xing, X. Wang, and J. H. Parks, Phys. Chem. Chem. Phys. 18 , 743 (2016). DOI:10.1039/C5CP06116D
[32] G. M. Koretsky, and M. B. Knickelbein, J. Chem. Phys. 107 , 10555 (1997). DOI:10.1063/1.474219
[33] L. Jiang, and Q. Xu, J. Phys. Chem. A 110 , 11488 (2006). DOI:10.1021/jp064129s
[34] H. Gronbeck, A. Hellman, and A. Gavrin, J. Phys. Chem. A 111 , 6062 (2007). DOI:10.1021/jp071117d
[35] J. Hagen, L. D. Socaciu-Siebert, J. Le Roux, D. Popolan, S. Vajda, T. M. Bernhardt, and L. Woeste, Int. J. Mass spectrom. 261 , 152 (2007). DOI:10.1016/j.ijms.2006.08.008
[36] Z. X. Luo, G. U. Gamboa, M. Y. Jia, A. C. Reber, S. N. Khanna, and A. W. Castleman, J. Phys. Chem. A 118 , 8345 (2014). DOI:10.1021/jp501164g
[37] X. Cao, M. Chen, J. Ma, B. Yin, and X. Xing, Phys. Chem. Chem. Phys. 19 , 196 (2017). DOI:10.1039/C6CP06741G
[38] J. Ma, X. Cao, L. Hao, Y. Baoqi, and X. Xing, Phys. Chem. Chem. Phys. 18 , 12819 (2016). DOI:10.1039/C6CP01156J
[39] J. Ma, X. Cao, M. Chen, B. Yin, X. Xing, and X. Wang, J. Phys. Chem. A 120 , 9131 (2016). DOI:10.1021/acs.jpca.6b09129
[40] A. D. Becke, J. Chem. Phys. 98 , 1372 (1993). DOI:10.1063/1.464304
[41] C. Lee, W. Yang, and R. G. Parr, Phys. Rev. B 37 , 785 (1988). DOI:10.1103/PhysRevB.37.785
[42] P. J. Stephens, F. J. Devlin, C. F. Chabalowski, and M. J. Frisch, J. Phys. Chem. 98 , 11623 (1994). DOI:10.1021/j100096a001
[43] K. L. Schuchardt, B. T. Didier, T. Elsethagen, L. Sun, V. Gurumoorthi, J. Chase, J. Li, and T. L. Windus, J. Chem. Inf. Model. 47 , 1045 (2007). DOI:10.1021/ci600510j
[44] M. J. Frisch, G. W. Trucks, H. B. Schlegel, G. E. Scuseria, M. A. Robb, J. R. Cheeseman, G. Scalmani, V. Barone, B. Mennucci, G. A. Petersson, H. Nakatsuji, M. Caricato, X. Li, H. P. Hratchian, A. F. Izmaylov, J. Bloino, G. Zheng, J. L. Sonnenberg, M. Hada, M. Ehara, K. Toyota, R. Fukuda, J. Hasegawa, M. Ishida, T. Nakajima, Y. Honda, O. Kitao, H. Nakai, T. Vreven, J. A. Jr. Montgomery, J. E. Peralta, F. Ogliaro, M. Bearpark, J. J. Heyd, E. Brothers, K. N. Kudin, V. N. Staroverov, R. Kobayashi, J. Normand, K. Raghavachari, A. Rendell, J. C. Burant, S. S. Iyengar, J. Tomasi, M. Cossi, N. Rega, N. J. Millam, M. Klene, J. E. Knox, J. B. Cross, V. Bakken, C. Adamo, J. Jaramillo, R. Gomperts, R. E. Stratmann, O. Yazyev, A. J. Austin, R. Cammi, C. Pomelli, J. W. Ochter-ski, R. L. Martin, K. Morokuma, V. G. Zakrzewski, G. A. Voth, P. Salvador, J. J. Dannenberg, S. Dapprich, A. D. Daniels, Ö. Farkas, J. B. Foresman, J. V. Ortiz, J. Cioslowski, and D. J. Fox, Gaussian 09, Revision A02, Wallingford, CT: Gaussian Inc., (2009).
[45] U. Burghaus, and H. Conrad, Surf. Sci. 364 , 109 (1996). DOI:10.1016/0039-6028(96)00601-2
[46] J. V. Barth, and T. Zambelli, Surf. Sci. 513 , 359 (2002). DOI:10.1016/S0039-6028(02)01780-6
[47] U. Burghaus and H. Conrad, Surf. Sci. 338, L869(1995).
[48] U. Burghaus, and H. Conrad, Surf. Sci. 201 , 352–354 (1996).
[49] A. F. Benton, and J. C. Elgin, J. Am. Chem. Soc. 48 , 3027 (1926). DOI:10.1021/ja01691a005
[50] R. J. Mikovksy, M. Boudart, and H. S. Taylor, J. Am. Chem. Soc. 76 , 3814 (1954). DOI:10.1021/ja01643a067
[51] A. L. de Oliveira, A. Wolf, and F. Schuth, Catal. Lett. 73 , 157 (2001). DOI:10.1023/A:1016641708074
[52] S. Klacar, and H. Grönbeck, Catal. Sci. Technol. 3 , 183 (2013). DOI:10.1039/C2CY20343J
[53] Z. P. Qu, W. X. Huang, M. J. Cheng, and X. H. Bao, J. Phys. Chem. B 109 , 15842 (2005). DOI:10.1021/jp050152m
银团簇上吸附氧原子与氢气作用的研究
曹西子, 殷保祺, 王亭亭, 邢小鹏     
同济大学化学科学与工程学院, 上海市化学品分析、风险评估与控制重点实验室, 上海 200092
摘要: 利用质谱实验和密度泛函理论(DFT)研究了AgnO-n=1~8)团簇与H2(或D2)的相互作用.质谱实验发现,150 K低温条件下所有AgnO-n=1~8)团簇中的氧原子与H2或D2作用时都呈现出惰性,这和之前研究发现的在同样条件下这些氧原子与CO作用中显现出的高活性形成鲜明对比.而这两者的鲜明对比与凝聚相中分散银体系的表现相一致,其能从氢气中选择性催化氧化痕量CO杂质.利用DFT方法计算了AgnO-n=1~8)团簇与H2作用的可能反应路径,理论结果表明H2在上述任一团簇的任一吸附位点的作用都很微弱,H2与上述团簇中任一氧原子的反应都有一个明显的势垒,其势垒高度与氧原子的吸附结构相关.上述这些实验观察和理论计算帮助从分子水平理解真实分散银催化剂表面原子氧物种的物理化学行为.
关键词: 银团簇    原子化氧    氢气    质谱技术    密度泛函理论计算