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CATALYST STRUCTURE STUDIED BY A LABORATORY EXAFS FACILITY : Ru/Al2O3

Y. Udagawa, K. Tohji, Z. Lin, T. Okuhara, M. Misono

To cite this version:

Y. Udagawa, K. Tohji, Z. Lin, T. Okuhara, M. Misono. CATALYST STRUCTURE STUDIED BY

A LABORATORY EXAFS FACILITY : Ru/Al2O3. Journal de Physique Colloques, 1986, 47 (C8),

pp.C8-249-C8-253. �10.1051/jphyscol:1986846�. �jpa-00226168�

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JOURNAL D E PHYSIQUE

Colloque C8, suppl6ment au no 12, Tome 47, decembre 1986

CATALYST STRUCTURE STUDIED BY A LABORATORY EXAFS FACILITY : Ru/A1203

Y. UDAGAWA, K. TOAJI, Z. Z. LIN*

( )

, T. OKUHARA" and M. MISONO*

Institute for Molecular Science, Okazaki, Aichi 444, Japan ' ~ e p a r t m e n t of Synthetic Chemistry, Faculty of Engineering, The University o f Tokyo, Bunkyo-ku, Tokyo 113, Japan

A laboratory EXAFS spectrometer is described which features the utilization of higher order reflections from curved dispersing crystal. With this spectrometer a sufficient performance for

structural analyses are obtained in the high energy region up to about 25 keV. It was applied to structurally characterize two kinds of Ru/AI2O3 catalysts, prepared from RuC13 and R U ~ ( C O ) ~ ~ , by the R u K EXAFS, combined with Hz adsorption and EM observations. I t was found

that Ru metal particles of different sizes were formed depending on the starting material and the procedure. In the catalyst prepared from R U ~ ( C O ) ~ ~ , small metal particles, possibly consist of about 20 atoms, are formed. They are small enough to show a contraction of the nearest neighbor distance by 0.06 A.

1 . l NTRODUCT 1 ON

Laboratory EXAFS spectrometers have advantages over synchrotron facilities in several respects; much faster and better interaction between the experiments and ideas, among others. In order to develop laboratory EXAFS facilities, a workshop was held in 1980 [ l l and the possibility to construct ones that can supply data accurate enough for structural analysis was discussed. Since then several laboratory spectrometers have been constructed by employing focused optics in order to compensate relatively weak x-ray intensity from conventional x-ray generators [ 2 - 5 1 . Some have already been utilized to

structurally characterize amorphous materials and liquids. All the studies so far reported, however, have been confined to the first raw transition elements only [ 6 - 1 1 1 , the reason being in poor resolving power at higher energy region

(

> I 5 kev).

In this study an improvement of the resolution in the high energy region has been attempted by the use of the higher order reflections from dispersing crystals. In order to discriminate unwanted

reflections which always accompany the desired one, a solid state detector was employed. As a result, a sufficient resolution as well a s photon numbers for EXAFS analysis was obtained for the energy range up to about 25 keV.

By the use of the spectrometer, structures of two kinds of

Ru/Al 0 catalysts, prepared from RuCl and R u (GO) , were studied by the RZ 2 EXAFS ( a b s o ~ p t i o n edge 22.14 f?e~). I? wasl?ound that very tiny metal clusters were formed in the catalyst prepared from R u (C0)12. They are so small that structural parameters differ

siinificantly from those of bulk metal; the coordination number is

(''present a d d r e s s : Department of Chemistry. Amoy University, F u j a n , China

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1986846

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C8-250 JOURNAL DE PHYSIQUE

about 6 instead of 12, the nearest neighbor distance contracts by 0.06 A compared to that of the bulk metal, and they are easily oxidized if kept in air at room temperature.

2. EXPER I MENTAL

The spectrometer employed is the one previously reported [ 5 1 . I t has a Rowland radius of 320 m and is equipped with a Johansson cut and bent crystal. X-rays from a rotating anode x-ray generator are monochromatized by either Ge(220) or Ge(311) dispersing crystal, and

the discrimination of the reflections by undesired orders is made by a combination of an SSD, and a 4 channel discriminator and scaler.

Photons from up to 4 different orders of reflection can be accumulated separately, and the desired one is picked out after transferred to a microcomputer through a CAMAC bus. photon numbers from all the orders less than 10 cps. I t was nece sary to maintain total 8 , in order to avoid a counting loss. This imposes a limitation to the available x- ray intensity. A use of aluminum foil filter was efficient for the elimination of lower order reflections. By the use of a rotating sample holder, I and I which are the x-ray intensities with a sample in and out of the beam!'were measured alternatively. Each abso ption measurement required about 12 hours, collecting at least 2 x 10 8

photons as I at each data point. EXAFS analysis was performed a s reported previously [7,8].

Ru/A1 0 catalysts were prepared by impregnating r-A1203 2 3

(Reference Catalyst of Catalysis Society of Japan, ALO-4) of a hexane solution of R u (CO)12 or aqueous solution of RuC13 as described previously [12Q. T h e former will be abbreviated as catalyst A and the

latter catalyst B. The contents of R u were 4 % in the former and 5 % in the latter. The catalysts in a glass cell with very thin wall were reduced by Hz at 450 C for 2 hrs. EXAFS measurements were performed with the sample sealed under vacuum after the reduction. In order to

study the effects of cxidation, the catalysts exposed to air at room temperature were also studied.

3. RESULTS

A n improvement of the resolving power by the use of higher order reflections is demonstrated in Fig. 1 , taking Mo K doublet as an example. Resolution (FWJ%M) of 7 eV at 18 k e ~ ' h : : ~ b : & attained with Ge(660) reflection, which is sufficient for EXAFS analysis.

Figure 2 shows EXAFS spectra of the R u catalyst A and B , a s well a s that of R u metal, taken with Ge(660) crystal. A comparison of the EXAFS function ~ ( k ) for R u metal and the two catalysts are shown in Fig. 3. It is evident from the figure that the ~ ( k ) of the catalyst B, which is prepared from RuCl,, almost coincides with that of the metal, except for a slightly fast

damping in the high k region. This indicates that R u atoms In the catalyst B are coordinated by other R u atoms in

the same way as in the bulk metal, possibly with a slightly larger disorder factor or with a smaller mean free path of the photoelectron. On the other hand, ~ ( k ) of the catalyst A , which is

prepared from R u (CO) , is

17.34 17.38 17.42 17.46 17.50

significantly dipfereh?; amplitude is

E N E R G Y / k e v

much smaller and the period is slightly

longer. From these qualitative Figure 1. Resolution of the observations a decrease in the monochromator by the use of

Ge(660) reflection.

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coordination number and shorter

1.5

nearest neighbor distance in the catalyst A can be anticipated.

Fourier transforms were mad7 over k range of 3.55 to 14.55 A followed by back-Fourier transforms of the first peak and the non- linear least-squares parameter fittings. The phase and amplitude factors reported by Teo and Lee

8.5

[13] were employed in the

calculation. The best fit values of the interatomic distances and

the catalyst B is predominantly

ENERGYCEU)

the coordination numbers are shown

a . 0

in Table I.

I t is concluded from the

metallic.- he interatomic distince is the same as that of the metal and the difference in the

coordination number is within the experimental error. Indeed, as is also shown in Table I , an

observation of electron microscope(EM) revealed the

presence of metal clusters with

-...>

. . . . . . . .2 :

.--... j i--.Jh

2 4 6

mean diameter of 71 A , whish is large enough to show no

significant surface effects.

On the other hand, the environment of R u atoms in the catalyst A is fairly different from that of the metal; the nearest neighbor distance is shorter by a s much as 0.06 A , and the coordi- nation number is almost the half.

N o observation of metal particles was made on this catalyst by EM, and X-ray diffraction(XRD) did not give any distinct peak. All these observations lead to the conclusion

results above that the R u atoms in

21750 22000 22250 22566 22750 23000 23250

Figure 2. EXAFS spectra of R u metal (M), catalyst A (from R u (CO)

) ,

and catalyst B (from I3u8l,).l2~he energies for A and B3are displaced. Inserted is a k weighted Fourier transform of R u metal (phase and amplitude uncorrected).

Figure 3. Extracted EXAFS oscillations of R u metal(dots),catalyst A (triangles), and catalyst B(so1id lines).

Table I. Characterization of Ru/A1 O3 catalyst prepared from Ru3(CO) (A) and from R~EI~(B).

Catalyst Diameter/(A) EXAFS DATA

HZ adsorption EM XRD A * I?"'

B(from RuC13) 4 6 7 1 nd* 2.65 11.0 Xi~nteratomic distance of Ru metal is 2.68 A.

*3Coordination number of Ru metal is 12.

Not detected.

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JOURNAL DE PHYSIQUE

that the Ru atoms in catalyst A exist in much smaller metal clusters than those of the catalyst B, resulting in the low coordination number and the shorter interatomic distance.

The changes in the EXAFS spectra when these catalysts were exposed to air give another clue to the understanding of the structure of these catalysts. As is shown in Fig. 4, EXAFS function of catalyst A after exposure to air becomes a single, monotonously decreasing oscillation with lower frequency, suggesting that the atoms

surrounding each R u atom are not Ru, but light atoms, and the oxygen is the only candidate in this case. In the Fourier transform of the extracted oscillation only one peak appears, which corresponds to Ru-0 distance. There also appears a sharp peak near the absorption edge, which is absent in metals and is often characteristic of the

absorption spectra of oxides. In the catalyst B, the metal like oscillation remains after the exposure to air as is shown in Fig. 5, but another oscillation with lower frequency is superposed. As a result, the associated Fourier transform shows two major peaks; one is Ru-Ru and the other is, most likely, Ru-0. All these evidences

suggest that metal atoms on the surface are easily oxidized by the exposure to air. Since the metal particle sizes in the catalyst A is so small almost all the R u atoms are oxidized, while in the catalyst B only those atoms on the surface are oxidized, the bulk remaining as metallic.

Figure 4. An EXAFS spectrum of catalyst A after expgsure to air and the associated k weighted Fourier transform (phase and amplitude uncorrected).

Figure 5. An EXAFS spectrum of catalyst B after expgsure to air and the associated k weighted Fourier transform (phase and amplitude uncorrected).

4. Discussion

EXAFS analysis of Ru/A1203 samples combined with EM, XRD, and H adsorption studies showed that depending on the preparation method, 8 u metal clusters of various sizes are formed. The metal particle size in

the catalyst B was determined by EM to be about 7 0 A, and the nearest neighbor distance and the coordination number obtained from EXAFS are almost the same as those of bulk metal in this case. The cluster size

in the catalyst A is, however, too small to be determined from EM, but the coordination number of 6 was obtained from EXAFS.

A rough estimation of the cluster size is possible from the

coordination number. Taking the hcp structure which bulk R u metal

assumes as a basis, two simple models that have the coordination

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number of about 6 can be conceived; an infinite two dimensional closed pack model gives the coordination number of 6 , and that of a hcp structure consisting of 20 atoms (three layers, with 5, 10, and 5 atoms in each layer) happened to be 6.3. The latter model is more likely to be close to the case, because the former requires fairly large number of atoms in order for the coordination number to be nearly 6. From the H adsorption study by assuming a cubic shape, the average half side of ?he particle was estimated to be about 10 A. 20 atom model fits this result, because it can be approximated to be an ellipsoid with diameters of about 11 and 7 A , which almost is

identical to a cube with half side of 10 A.

Another interesting result is the considerable contraction of the nearest neighbor distance in catalyst A. Contractions due to surface stress can be expected for very small particles and several examples have already been reported. Montano et al. [14] reported a decrease of about 0.04 A in the nearest neighbor distance of Ag particles in solid argon with average sizes ranging from 25 to 150 A. In a

separate publication they observed a significant contraction of Fe-Fe distance, although the particle size was not known [15]. Moraweck et al. [I61 have reported a contraction of Pt-Pt distance by 0.12 A in a Pt/Y-zeolite sample. The observation here has added another evidence that the contraction does occur in very small particles.

Asakura et a1.[17] studied the structure of Ru/T-A1203 and Ru/Si02 prepared from R U ~ ( C O ) ~ ~ by EXAFS and observed Ru-0 bond as well as Ru-Ru bond (2.64 A) for Ru/Al 0 . They attributed the Ru-0 bond to

the one between the metal and2tfie surface oxygen of the support. In the result presented here, no evidence for Ru-0 bond was obtained with the sample kept in vacuo after reduction. The reason of the

discrepancy is not known at this point.

References

1. American Institute of Physics Conference Proceedings N0.64, Edited by E.A.Stern (American Institute of Physics, New York, 1980).

2. S.Khalid, R.Emrich, R-Dujari, J.Schultz, and J.R.Katzer, Rev.

Sci. Instrum. 53, 22 (1982).

3. A.Williams, Rev. Sci. Instrum. 54, 193 (1983).

4. W.Thulke, R.Haense1, and P.Rabe, Rev. Sci. Instrum. 54, 277(1983).

5. K.Tohji, Y.Udagawa, T.Kawasaki, and K.Masuda, Rev. Sci. Instrum.

54, 1482 (1983).

6. W.Thulke, R.Haense1, and P.Rabe, Phys. Stat. Solid 78, 539 (1983).

7. K.Tohji, Y.Udagawa, S.Tanabe, and A.Ueno, J. Am. Chem. Soc. 106, 612 (1984).

8. K.Tohji, Y.Udagawa, T.Ida, S.Tanabe, and A.Ueno, J. Am. Chem. Soc.

106, 5671 (1984).

9. F.G.Halaka, J.J.Boland, and J.D.Baldschwieler, J. Am. Chem. Soc.

106, 5408 (1984).

10. K.Ozutsumi, T-Yamaguchi, H.Ohtaki, K.Tohji, and Y.Udagawa, Bull.

Chem. Soc. Jpn. 58, 2786 (1985).

11. K.Tohji, Y.Udagawa, T.Mizushima, and A.Ueno, J. Phys. Chem. 89, 5671 (1985).

12. T-Okuhara, T.Kirnura, K.Kobayashi, M.Misono, and Y-Yoneda, Bull.

Chem. Soc. Jpn. 57, 938 (1984).

13. B.K Teo and P.A.Lee, J. Am. Chem. Soc. 101, 2815 (1979).

14. P.A.Montano, W.Schultze, B.Tesehe, G.K.Shenoy, and T.I.Morrison, Phys. Rev. B30, 672 (1984).

15. H.Purdun, P.A.Montano, Q.K.Shenoy, and T.Morrison, Phys. Rev. B25, 4412 (1982).

16. B.Moraweck, G.Clugnet, and A.J.Renouprez, Surf. Sci. 81, L631(1979).

17. K.Asakura, M-Yamada, Y.Iwasawa, and H.Kuroda, Chem. Lett. 1985,

511 (1985).

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