Infrared Reflection Absorption Spectroscopy (IRRAS) of Ethene

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Aug 17, 2010 - of Ethene (C2H4) Chemisorbed on the Bare and Roughened. Cu(110) and Cu(111) ..... Formation of ethylene dimers. Spectrochimica Acta ...
O 36.24: Infrared Reflection Absorption Spectroscopy (IRRAS) of Ethene (C2H4) Chemisorbed on the Bare and Roughened Cu(110) and Cu(111) Surfaces Jan Pischel, Olaf Skibbe, and Annemarie Pucci

Kirchhoff-Institut für Physik Im Neuenheimer Feld 227 D-69120 Heidelberg

U NIVERSITÄT H EIDELBERG

Introduction

IRRAS

AlAlAl Al AlAlAlAlAl Al Al Al AlAl AlAlAl AlAlAlAl Al Al Al Al Al AlAlAl Al AlAl AlAlAlAlAl Al Al Al Al Al AlAl AlAl AlAl Al AlAlAlAlAl Al Al AlAlAlAlAl AlAlAl AlAlAl Al Al Al Al Al Al AlAlAlAl AlAlAlAlAlAlAl Al AlAlAl Al Al Al Al Al Al AlAlAl Al AlAlAl AlAlAlAlAl Al Al AlAl AlAlAl AlAlAl Al AlAlAlAlAlAl Al AlAl Al Al AlAlAlAl Al Al Al AlAl AlAl Al AlAlAl Al AlAl Al Al AlAl Al Al

[110]

ˆ incoming p-polarized IR-beam (diameter ≈ 2 mm) near gracing incidence (θ ≈ 85°) reflected by metal surface

Tab. 1: Some of the normal modes of gas phase ethene (nomenclature according to ref. [6]). Obeying the Raman-IR exclusion principle, the modes are either Raman active (R), infrared active (IR) or silent (s). The corresponding frequencies of solid ethene and of ethene adsorbed on the Cu(110) and Cu(111) surfaces are given in cm−1. mode

ν2

ν3

ν7

ν8

ν10

ˆ reference spectrum: smooth or roughened surface, bare

of adsorbates

ν12

ˆ only IR-active vibrations of adsorbates with dynamic

dipole moment perpendicular to the surface may be excited

visualization [6]

[001]

name activity frequency (solid) [7]

Fig. 1: The highly anisotropic Cu(110) surface (left) and the close-packed Cu(111) surface (right). Images generated by [1].

As a model for an organic-metal interface, the chemisorption systems C2H4/Cu(111) and C2H4/Cu(110) have attracted attention because of their remarkable absorption properties in infrared (IR) spectroscopy [2, 3, 4, 5]. Not only were two gas phase Raman active modes observed that are expected to be IR forbidden by the Raman-IR exclusion principle for centrosymmetric molecules, but also the only IR active mode allowed by the metal surface selection rule seemed to disappear at higher coverages on Cu(110). No final conclusion concerning these findings has been drawn so far. This brought us to reinvestigate the system C2H4/Cu(110) by means of IRRAS.

CC-stretch CH2-deformation CH2-wagging CH2-wagging CH2-rocking CH2-deformation R R IR R IR IR 1615, 1622 1329, 1348 942, 951 942, 952 820, 826 1436, 1440 C2H4/Cu(110) low coverage 1532, 1552 high coverage 1522 low coverage high coverage 1522 1534 low coverage 1535 high coverage 1523 ice layer 1518

ref.[2] ref.[3] ref. [4] this work

1274, 1285 1261 1275 1257 1275 1275 1260 1256

916 906 904 907 850 847, 957

-

821

1440

evaporator Omicron EFM3

1535 1539

sputtergun: Ar+ , 2 keV

UHV: p ≤ 6·10-11 mbar gases: C2H4 , CO, O2, ...

FTIR-spectrometer

1285 1283

910 916

-

-

QMB

40K ≤ T ≤ 900K

C2H4/Cu(111) ref. [8] ref. [9]

sample

IRRAS

-

detector

Fig. 2: Experimental setup.

C2H4/Cu(110) 1.9 L

1519 c

c

887

99,0

0.67 L

1.00 L

0.51 L 0.58 L

c c

c

c

98,5

1.67 L

1550

957

CC-stretch

0.30 L

0.44 L

[%] 0

rel. reflectance R/R

1535

1275

0

907

1440

c

rel. reflectance R/R

0.16 L 99,5

1560

c

annealed

1256

1540

1530 1523

1520 c

1.91 L

c

0.2 %

1260

98,0

1500

1600

-1

800

900

1000

1200

1300

1400

1500

wavenumber [cm ]

1600

-1

wavenumber [cm ]

Fig. 3: IRRAS spectra of C2H4/Cu(110) at 60 K and different exposures. The plane of incidence is oriented parallel to the [1¯10] direction. With increasing exposures, the Raman active modes develop and shift to lower frequencies whereas the IR active mode broadens significantly. At exposures higher than 1.4 Lc, multilayer adsorption occurs (ice peak at 957 cm−1).

Fig. 5: IRRAS spectra of 1.9 Lc C2H4/Cu(110) at 50 K before and after annealing to 90 K for 100 s. The ice layer desorbs and the Raman active modes become sharper and deeper. 0.00 ML

1290

0.18 ML

1280

1270

2

1400

CH -scissors

1300

-1

1200

peak position [cm ]

1256

957

800 850 900 950 1000

1519

1260

0.5 % 1521

rel. reflectance R/R

960

0.12 ML

940

0.18 ML 0.23 ML 0.5 ML

920

900

3.0 ML

800

900

1000

1200

860

1300

0.2 %

880

1544

1277

894

1440 1518

all surfaces

2

0

c

4.2 ML

821 847

smooth surfaces

860

CH -wagging

average

rel. reflectance R/R

0.035 ML

rough surfaces

0

07/29/10

93 L

1258

[%]

08/17/10

1400

1500

1600

0,0

0,5

1,0

1,5

2,0

-1

957

wavenumber [cm ]

1256

dose [L ] c

800

1000

1200

1400

1600

-1

wavenumber [cm ]

Fig. 4: IRRAS spectra of 1.9 Lc C2H4/Cu(110) at about 50 K measured at two different days and their average (baseline corrected). The detail of a spectrum with very high exposure (93 Lc) is shown in order to identify the origin of the mode at 821 cm−1.

Fig. 6: IRRAS spectra of 1.9 Lc C2H4/Cu/Cu(110) at 50 K after annealing to 90 K for 100 s for various amounts of cold-evaporated copper. The quantity of evaporated atoms is given in units of monolayers (ML), where 1 ML represents the number of atoms within one atomic layer (although layer-by-layer growth is not necessarily taking place). With increasing surface roughness, the Raman peaks split up and the IR active mode appears near 900 cm−1.

Conclusions

C2H4/Cu(111) -1

Wavenumber [cm ] 0

1000

2000

3000

4000

0.00 ML

-1

115meV (920cm )

0.2 %

0.97 ML 1.3 ML

x300

800 850 900 950 1000

1200

1508

1300

1400

specular

1543

1500

erage on Cu(110) but appears to become broader and broader until it almost gets lost in the noise. Cu(110) and Cu(111) surfaces differ strongly: On Cu(110), the most prominent features are the IR forbidden Raman active modes ν2 and ν3, whereas on Cu(111) those modes are hardly distinguishable and the IR active mode is clearly visible.

off-specular

1.8 ML

1280

381meV(3048cm-1)

x300

371meV (2968cm-1)

0.64 ML

7meV

258meV (2064cm-1)

0.39 ML

230meV (1840cm-1)

0.23 ML

196meV (1568cm-1)

157meV (1256cm-1)

1551

intensity [a.u.]

rel. reflectance

0.04 ML

1241

ˆ The IR-active mode ν7 does not really disappear with increasing cov-

ˆ The spectra obtained for saturation coverage C2H4 on the bare

1284

915

Fig. 7: Schematic represantation of the dependence of the observed ethene peak positions on surface roughness and ethene exposure. The bars show the trend derived from several hundred spectra. Surfaces with less than 0.18 ML copper evaporated show similar properties, can be pooled and are called “smooth”. Analogously, those with higher amounts of cold-evaporated copper are called “rough”.

1600

-1

wavenumber [cm ]

0

100

200

300

400

500

Energy loss [meV]

Fig. 8: IRRAS spectra of C2H4/Cu/Cu(111) at saturation coverage (T = 95 K) for various amounts of cold-evaporated copper. Data taken from [5, 9], new compilation.

Fig. 9: High resolution electron energy loss (HREEL) spectra of 1.1 Lc C2H4/Cu(111) at 85 K (comparison between specular and 10° off-specular geometry) [5, 9].

References

[3] Kubota, J., J. N. Kondo, K. Domen, and C. Hirose: IRAS Studies of Adsorbed Ethene (C2H4) on Clean and Oxygen-Covered Cu(110) Surfaces. J. Phys. Chem., 98:7653-7656, 1994.

[1] Hermann, K. and F. Rammer: surface explorer. http://surfexp. fhi-berlin.mpg.de. [2] Jenks, C. J., B. E. Bent, N. Bernstein, and F. Zaera: Evidence for an unusual coordination geometry for ethylene on Cu(110). Surf. Sci. Lett., 277:L89-L94, 1994.

[4] Raval, R.: Probing the nature of molecular chemisorption using RAIRS. Surf. Sci., 343:201-210, 1995. [5] Skibbe, O., M. Binder, A. Otto, and A. Pucci: Electronic contributions to infrared spectra of adsorbate molecules on metal surfaces: Ethene on Cu(1 1 1). J. Chem. Phys., 128:194703-1 - 194703-6, 2008.

ˆ The intensity of ν2 and ν3 on Cu(110) is stronger or at least com-

parable with that of the IR-active mode ν7 on Cu(111). This could be explained if the modes of the adsorbed molecule on Cu(110) were found to possess a dynamic dipole moment. ˆ Upon roughening the surfaces, their adsorption properties concerning

ethene become similar as might be expected considering the fact that the single crystalline surfaces get covered and the same kind of defects govern the surface properties.

[6] Herzberg, G.: Infrared and Raman Spectra of Polyatmic Molecules. D. van Nostrand Company, Princeton, Reprint 1964. [7] Rytter, E. and D. M. Gruen: Infrared spectra of matrix isolated and solid ethylene. Formation of ethylene dimers. Spectrochimica Acta, 35A:199-207, 1979. [8] McCash, E. M.: 1989 C. R. Burch Prize: Surfaces and vibrations. Vacuum, 40(5), 1990. [9] Binder, M.: Untersuchung von Ethen auf der glatten und aufgerauten Cu(111)-Oberfl¨ache mit IRRAS und HREELS. Diploma Thesis, University of Heidelberg, 2006.