on Ultrathin MgO Films Grown on a Mo(ll0) - American Chemical Society

Department of Chemical Engineering and Materials Science, University of California, Davis, California 9561 6, and Department of Chemistry, Texas A&M U...
1 downloads 10 Views 795KB Size
J . Phys. Chem. 1994,98, 4076-4082

4076

Adsorption and Reaction of [Re2(CO)lo] on Ultrathin MgO Films Grown on a Mo(ll0) Surface: Characterization by Infrared Reflection-Absorption Spectroscopy and Temperature-Programmed Desorption S. K. Purnell,t X. Xu,* D. W. Goodman,'** and B. C. Gates'9t Department of Chemical Engineering and Materials Science, University of California, Davis, California 95616, and Department of Chemistry, Texas A&M University, College Station, Texas 77843 Received: October 19, 1993; In Final Form: January 31, 1994"

The decarbonylation of [Rez(CO)lo] on ultrathin MgO( 111) films (-50 A) grown on a Mo( 110) substrate was investigated with infrared reflection-absorption spectroscopy and temperature-programmed desorption/ decomposition. When [Re2(CO)lo] was adsorbed at 320 K, it reacted with the M g O ( l l 1 ) surface, forming a rhenium subcarbonyl, [Re(CO)4{OMg}12,where {OMg] represents oxygen on the M g O ( l l 1 ) surface. Upon heating to temperatures >400 K, [Re(C0)4{OMg}]2 was decarbonylated, forming [Re(CO)3{OMgJ3]. Further heating to temperatures >600 K induced the formation of rhenium metal clusters. When it was adsorbed at 110 K, [Re2(CO)lo] condensed on MgO( 1I l), with a fraction of the first layer decomposing to form [Re(C0)4{0Mg}]2. In temperature-programmed desorption experiments, [Re2(CO)lo] multilayers desorbed at 295 K. An unidentified rhenium carbonyl species, probably rhenium pentacarbonyl, desorbed at 350 K. The C O stretching frequencies of the rhenium subcarbonyls were dependent on the coadsorption of water. The infrared spectra show that the symmetry of the surface-bound rhenium tricarbonyls is C3". The results are among the first characterizing the adsorption of metal complexes on well-defined metal oxide surfaces, and they demonstrate the value of structurally characterized supports for elucidation of the nature of the metal-support interface.

Introduction Supported metal catalysts are extremely important in technology, but their structures are not well understood because the metal clusters or crystallites are highly nonuniform in size and shape and the suppoft surfaces are heterogeneous. In attempts to understand the structure of the metal-support interface better, experiments have been done with simple mononuclear (singlemetal-atom) complexes bonded to the surfaces of metal oxide powders.'" Their structures have been characterized with a variety of techniques, including infrared spectroscopy, temperature programmed desorption/decomposition (TPD), and extended X-ray absorption fine structure (EXAFS) spectroscopy. Models have been proposed for these structures, accounting for both metalCO bonding and metal-support bonding. However, the surfaces of the metal oxide powders are highly nonuniform, and the available physical data provide only average structural information. Thus, the identities of the crystal planes on which the structures are bonded are unknown, and the possibility that the structures exist largely at defect sites has been virtually impossible to assess.5 The goals of this work were to prepare rhenium subcarbonyls like those described above on a relatively well-definedmetal oxide surface under ultrahigh-vacuum conditions. [Re*(CO)101 was chosen to be the organometallic precursor because it has been shown to lead to well-defined structures on MgO powdersSand has a vapor pressure high enough to allow for vapor deposition in ultrahigh-vacuum apparatus. The surface was chosen to be that of a MgO thin film because thin MgO films can be easily prepared and characterized with an array of surface science techniq~es.~JThin films on metal single crystals are more attractive than bulk metal oxide single crystals because they are good conductors and can be more easily cleaned, cooled, and reheated than the bulk insulating materials, and they do not become charged as bulk metal oxides do in experiments carried t University of California. f @

Texas A&M University. Abstract published in Advance ACS Abstracts, March 15, 1994.

out with impinging beams of charged particles. Because the aforementioned rhenium subcarbonylS has C3, symmetry, the MgO thin films werechosen to be MgO( 11l), which, fortunately, can be grown on a Mo( 110) substrate. The samples were characterized by temperature-programmed desorption/decomposition (TPD) and infrared reflectionabsorption (IRAS) spectroscopybecause the results allow a direct comparison with results characterizing the powder samples.

Experimental Methods The TPD and IRAS experiments were performed in an ultrahigh-vacuum chamber described previo~sly.~ This chamber is equipped with Auger electron spectroscopy, a UTI mass spectrometer, and a Mattson Cygnus 100 FTIR spectrometer. The characterization of the MgO films was done in a separate chamber equipped with X-ray photoelectron (XPS), Auger electron (AES), and ion scattering (ISS) spectroscopiesand lowenergy electron diffraction (LEED). Identical procedures were used to prepare the MgO films in the two chambers. The base pressure of each chamber was < I t 9 Torr. Preparationand Characterizationof Ultrathin MgO( 11 1 ) Film on a Mo(ll0) Substrate. Thin MgO films were prepared by evaporating pure metallic magnesium in 5 X le7 Torr of oxygen (02) onto a clean Mo( 110) substrate at room temperature; the samples were subsequently annealed to 800 K. This method is similar to thatused toprepareMgO( 100) on Mo(100).*0 Mo(l10) was cleaned by heating in oxygen at 1200 K and flashing to 2000 K in uacuo. The MgO films were characterized by LEED and He+ ISS. LEED exhibited a good (1 X 1) hexagonal pattern, demonstrating (1 11) orientation of the MgO films. XPS and AES showed the film to have the stoichiometry of MgO and the absence of the Mgostate. ISS showed the surface to be composed of both oxygen and magnesium. The stability of the MgO films was investigated with temperature-programmed desorption; the films were found to be stable at temperatures C1400 K, and at higher temperatures the MgO was reduced by the Mo substrate, forming volatile Moos and Mg vapor.11 The MgO films used in this investigation were approximately 50 A thick.

0022-3654/94/2098-4076$04.50/00 1994 American Chemical Society

The Journal of Physical Chemistry, Vol. 98, No. 15, 1994 4077

[Rez(CO)lo] on Ultrathin MgO Films

Materials. [Rez(C0)10](Strem) was used as received. Before being admitted to the vacuum chamber, it was subjected to several freeze-pumpthaw cycles to completely remove any residual contaminants such as solvents used in the synthesis. The purity of the [Rez(CO)lo] was verified by mass spectrometry. Dosing of Rhenium Carbonyl onto the Surface. [Re2(CO)lo], having a vapor pressure of roughly a milliTorr, was introduced into the ultrahigh-vacuum system through a heated dosing line (-320 K) ending with a nozzle inside the main chamber. The flux was monitored by a mass spectrometer mounted in line with the dosing line. In general, the MgO surface was held at temperatures 400 K resulted in two major bands at 2058 and 1942 cm-1. Temperature-ProgrnmmedDesorptionof Samples Prepared by Adsorption of [Re2(CO)lo] at 320 K. Figure 4 shows the CO evolution during temperature-programmed desorption following saturation exposure of [ R ~ Z ( C O ) ,at~ ]room temperature. CO desorbed at 550 K, -70 K higher than the temperature of desorption of CO when the [Re2(CO)lo]had been adsorbed at 110 K. Infrared Reflection-Absorption Spectra of Samples Prepared by Adsorption of [Re2(CO),o] at 320 K. After exposing the MgO film to [Rez(CO)lo]vapor (exposure - 5 monolayers) at 320 K, the infrared spectra exhibited four well-resolved bands, at 2108, 2043, 2004, and 1958 cm-1 (Figure 5). When the sample was

300

500

700

900

Temperature (K) Figure4. Temperature-programmeddesorptionspectra for [Rez(CO)lo] on a MgO film. The adsorption temperature was 320 K. No rhenium carbonyl species were observed to desorb from this sample. heated to 400 K, the bands at 2108, 2043, and 2004 cm-I disappeared, and a new band emerged at 2052 cm-I. Further increases in the temperature led to decreased intensities of the bands at 2052 and 1935 cm-1 and also led to shifts of these bands to lower frequencies. Preadsorption of Water. Approximately 2 monolayersof water was introduced onto the MgO thin film at 110 K, followed by the adsorption of [ R ~ ~ ( C O ) I OBoth ] . the TPD and infrared data were nearly identical to the data characterizing samples prepared by adsorption of [Re2(CO)lo] in the absence of water (data not shown). However, the final rhenium coverage following [Rez( C O ) l ~decomposition ] on the water-precoveredsurface was only approximately half of that observed following decomposition of [Re2(CO)lo]adsorbed onto a clean MgO film. Multilayer water

The Journal of Physical Chemistry, Vol. 98, NO. 15, 1994 4079

[Re2(CO)l~] on Ultrathin MgO Films

-

IRAS, [Re(CO)51,/MgO/Mo(l 10) Tads-320 K 0.001 1958

2108

8

es 8 9

back to higher frequencies (Figures 6C,D). After the sample had been heated to 300 K400K

0

-co >600 K

Figure 7. Reaction scheme proposed for [Rez(CO)lo] on MgO(111)/ Mo( 110) following adsorption at 320 K. These bands are again attributed to rhenium subcarbonyls formulated as [Re(CO)3(OMg)3] because the observed band locations are nearly identical to those observed for the sample prepared by adsorption of [ R ~ Z ( C O )at~320 ~ ] Kafter it had been heated to 400-500 K. The broadness of the spectral features at 2054 and 1933 cm-I may be an indication of the presence of other minor surface species. Evidence of Metallic Rhenium Clusters. When the samples prepared from [ R ~ Z ( C O ) ,on ~ ] MgO films were heated to temperatures >700 K, nearly all the C O had been desorbed from the surface, as evidenced by temperature-programmed desorption and infrared spectra. The broad feature in the TPD spectrum (Figure 1B) in the temperature range 700-1000 K suggests that small amounts of CO dissociated on the surface and eventually recombined. The amount of CO dissociation increased with rhenium coverage (data not shown). The total amount of rhenium metal left on the MgO surface depended on the initial [ReT ( C O ) l ~coverage, ] with a maximum of -1 X 10'5 atoms/cm2. Proposed Reaction Schemes. In summary, a reaction scheme that accounts for the observations for [Re2(CO)lo] on MgO following adsorption at 320 K is shown in Figure 7. There is no evidence of intermediates in the decarbonylation of [Re(CO)3(OMg}3], A scheme representing the observationsfor the samples prepared by adsorption of [ReZ(CO)lo] at 110 K is more complicated. When [Re2(CO)lo] was adsorbed on MgO at 110 K, only a fraction of the molecules were decarbonylated, forming [Re(CO)4(OMg)]2.Thedegreeof decarbonylation increasedwith temperature. Multilayers of [Re2(CO)lo] desorbed at -295 K as other rhenium carbonyl species formed. Upon further heating to temperatures >300 K, [Re(CO),(OMg)2] and other unidentified speciesreacted to yield volatile rhenium carbonyls and surfacebound rhenium subcarbonyls such as [Re(C0)3(0Mg)3]. When the sample was heated to temperatures >600 K, metallic rhenium formed on the MgO surface. Effect of Preadsorbed Water. Since most powder metal oxide supports contain surface hydroxyl groups, whereas the MgO thin film did not, we preadsorbed water on the MgO film to examine its effect on the chemistry of the rhenium carbonyls. Both the TPD and infrared data characteristic of a sample prepared by adsorption of [ReZ(CO)101 on a MgO thin film that was precovered with water (-2 monolayers) were observed to be nearly the same as the corresponding data characterizing samples prepared by adsorption of [Re2(CO),o] on a MgO thin film in the absence of water. The similarity of the data suggests that samples prepared by adsorption of water before the adsorption of [Re~(CO)lol underwent surface reactions similar to thoseobserved for samples without water. However, the final rhenium coverage following decomposition of [Re2(CO)lo] on the water-precovered surface was only approximately half of the that observed for the sample without water. We speculate that the water (and possibly surface hydroxyl groups formed from it by reaction with the MgO) inhibited the adsorption of [ R ~ Z ( C O ) and , ~ ] its reaction with the MgO film.

Effect of Postadsorbed Water. Since the locations of the YCO bands of the surface-bound rhenium tricarbonyl have been reported to be sensitive to the degree of hydroxylation of the metal oxide powder surfaces,S.6 experiments were done to investigate theeffects ofwater adsorbedon theMgO film. Water was adsorbed after the adsorption of [Re~(CO)loland its subsequent conversion into surface-bound rhenium subcarbonyl species [Re(CO)3(OMg]3] by heating to 500 K. Prior to the adsorption of water, two uco bands were observed, at 2054 and 1934 cm-1 (Figure 6A). After adsorption of -2 monolayers of water at 100 K, the uco bands shifted to lower energies, 2024 and 1906 cm-1 (Figure 6B). These bands are close in their positions to the bands characterizing the rhenium subcarbonyls supported on MgO powder, the surface of which was estimated to be 93% dehydroxylated.6 Nature of the Bonding of the Rhenium Subcarbonyls to the MgO Surface. All the results are consistent with the formation of rhenium subcarbonyls having the composition [Re(C0)3(OMg)3]as a result of heating the samples to temperatures >400 K. The MgO film was epitaxially grown on Mo( 110) and had the hexagonal orientation of MgO( 111). Thus, the surface oxygen atoms were arranged in triangular arrays so that each of the three oxygen atoms in a triangle could readily bond as a ligand to a single rhenium atom in a metal complex such as [Re(C0)3(OMg)3],which is expected to have C3,symmetry and be analogous to numerous known molecular c o m p l e ~ e s . ~ ~ The intensity of the 2050-cm-*band was observed to be much stronger than that of the 1930-cm-I band for [Re(C0)3(0Mg]3] on the MgO thin film, whereas the opposite was true on MgO p o ~ d e r . ~Assuming C3, symmetry, the 2050-cm-I band is attributed to the symmetric stretching of the [Re(CO)3] group and has a dipole moment nearly perpendicular to the plane in which the three lattice oxygens lie, whereas the 1930-cm-I band is attributed to the antisymmetric motion and has its dipole moment nearly parallel to the MgO( 111) surface. Since IRAS can only probe vibrational modes having a perpendicular component because of the selection rule, the relative intensities of the bands at 2050 and 1930 cm-*further support the postulated structure of [Re(C0)3(0Mg}3]in which the [Re(CO)3] moiety is coordinated by three lattice oxygens and has C3, symmetry. This inference about the symmetry of the surface-bound rhenium subcarbonyls is in agreement with the conclusionsbased on EXAFS, infrared, and other evidence for rhenium tricarbonyls on the surface of MgO powder. However, the predominant face on MgO powder is the square (100) face, and the simplified structural models suggested for rhenium subcarbonyls on the MgO powder2"J9 are constrained by the incorporation of three surface oxygen atoms arranged in a square array. The misfit in these simplified models has led to the suggestion that the rhenium subcarbonyls were actually bonded at surface defect sites where their 3-fold symmetry could be accommodated in an energetically more favorable ways5 The present results add support to this suggestionand demonstrate thevalue of structurally characterized supports such as that used in the present work for elucidation of the nature of the metal-support interface. Conclusions [ R e ~ ( C 0 ) ~reacted o] with the MgO( 111) surface upon adsorption at 320 K, forming a surface-bound rhenium tetracarbonyl species, [Re(CO)4{OMg}]z. When the sample was heated to temperatures >400 K, [Re(CO)4{OMg)]2was decarbonylated, forming a surfacebound rhenium tricarbonyl, [Re(CO)3(OMg)3]. Further heating to temperatures >600 K induced the formation of rhenium metal clusters. Rhenium subcarbonyls were not reformed when the rhenium metal clusters were exposed to lowpressure CO at room temperature. When adsorbed at 110 K, [Re2(CO)lo] formed multilayers on MgO( 111) with a fraction of the first layer decomposing to form [Re(CO)4(OMg)]~.[Rez-

4082 The Journal of Physical Chemistry, Vol. 98, No. 15, 1994

(CO)IO]multilayers desorbed at 295 K. An unidentified rhenium carbonyl species, probably rhenium pentacarbonyl, was also desorbed at 350 K during temperature-programmed desorption experiments. Heating of the sample to40G500 K resulted in the formation of surface-bound rhenium tricarbonyls, [Re(C0)3(OMg)3]. The vco band frequencies of the rhenium subcarbonyl species were found to be dependent on the coadsorption of water. The infrared spectra show that the symmetry of the surfacebound rhenium tricarbonylsis C3". The conclusion is in agreement with the evidence chamcterizing rhenium tricarbonyls on MgO powder surfaces, which are predominantly MgO( 100). The results suggest that the rhenium subcarbonylsare bonded to defect sites or faces other than the (100) face on the powders. The results demonstrate the value of structurally characterized supports such as that used in the present work for elucidation of the nature of the metal-support interface.

Acknowledgment. This work was supportedby the Department of Energy, Office of Energy Research, Office of Basic Energy Sciences, Division of Chemical Sciences, Contract FG0588ER13954 at Texas A&M University and Contract FG0287ER13790 at the University of California at Davis. References and Notes (1) McKenna, W. P.;Higgins, B. E.; Eyring, E. E. J. Mol. Carol. 1985, 31, 199.

Purnell et al. (2) Kirlin, P. S.;DeThomas, F. A.; Bailey, J. W.; Gold, H. S.;Dybowski,

C.; Gates, B. C. J. Phys. Chem. 1986, 90,4882.

(3) van Zon, F. B. M.; Kirlin, P. S.;Gates, B. C.; Koningsberger, D.C. J . Phys. Chem. 1989, 93, 2218. (4) Kirlin, P.S.;van Zon, F. B. M.; Koningsberger, D.C.; Gates, B. C. J. Phys. Chem. 1990,94, 8439. (5) Papile, C. J.; Gates, B. C. hngmuir 1992, 8, 74. (6) Honji, A.; Gron, L. U.; Chang, J.-R.; Gates, B. C. hngmuir 1992, 8, 2715. (7) Xu,X.;Goodman, D.W. Surf.Sci. 1993,284, 103. (8) Xu, X.;Goodman, D.W. J . Phys. Chem. 1993,97,683. (9) Leung,L.-W.; He. J.-W.;Goodman, D.W. J. Chem. Phys. 1990,93, 8328. (10) Wu, M. C.; Corneille, J. S.;Estrada, C. A.; He, J. W.; Goodman, D. W. Chem. Phys. Lerr. 1991, 182, 472. (11) Xu,X.;Goodman, D.W. Manuscript in preparation. (12) Baev, A. K.; Dem'yanchuk, V. V.; Mirzoev, G.; Novikov, G. I.; Kolobova, N. E. Russ. J. Phys. Chem. (Engl. Transl.) 1971, 45, 777. (13) Adams, D.M.,Hooper, M. A. J. Organomer. Chem. 1979,181,131. (14) Cotton, F. A.; Wing, R. M. Inorg. Chem. 1965, 4, 1328. (15) Flitcroft, N.; Huggins, D.K.; Kaesz, H. D.Inorg. Chem. 1964, 3, 1123. (16) Adams, D.M.; Taylor, I. D. J. Chem. SOC.,Faraday Trans. 2 1982, 78, 1065. (17) Hileman, J. C.; Huggins, D.K.; Kaesz, H. D.Inorg. Chem. 1962,1, 933. (18) Bolivar, C.; Charmset, H.; Frety, R.; Primet, M.; Tournayan, L.; Betizeau, C.; Leclerq, G.; Maurel, R. J. Carol. 1976, 45, 163. (19) Chang, J.-R.; Gron, L. U.; Honji, A,; Sanchez, K. M.; Gates, B. C. J. Phys. Chem. 1991, 95,9944.