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Photoabsorption Spectroscopy at medium Resolution. The C2HXYZ (XYZ= H, F, Cl and/or Br) Molecules.

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PHOTOABSORPTION SPECTROSCOPY AT MEDIUM RESOLUTION . THE C2HXYZ (X,Y,Z = H, F, Cl and/or Br) MOLECULES.

R. Locht1, B. Leyh1, H.W. Jochims2 and H. Baumgärtel2.

1

Département de Chimie, Université de Liège, Institut de Chimie, Bât. B6c, Sart-Tilman par B-4000 Liège 1, Belgium.

2

Institut für Physikalische Chemie, Freie Universität Berlin, Takustrasse 3, D-14195 Berlin, Germany.

Since several years we proceed with the systematic investigation of halogenated derivatives of ethylene (C2H4). The photoabsorption and/or the photoionization of C2H3F and 1,1-C2H2F2 [1], C2H3Cl [2,3] and C2H3Br [4,5] has been studied. The dissociaton dynamics of the C2H3F+, 1,1-C2H2F2 + [1] and C2H3Br+ [6] cations were investigated. The photoabsorption and photoionization spectroscopy of C2H2Cl2 [7] and C2H2FCl [8] have also been examined by synchrotron radiation. Recently, the photodissociation of the cations and the kinetic energy distribution of the most abundant fragments have been measured by fixed wavelength photoionization (HeI, NeI and ArI/ArII resonance lines) in our laboratory.

We already mea-sured the threshold- (TPES) and HeI-photoelectron spec-tra of the last mentioned compounds. The photoab-sorption spectra recorded earlier with the 1.5m-NIM monochromator at BESSY I were of to low resolution. The aim of this work was to obtain the desired reso-lution, i.e. at least com-parable to that obtained in the TPES spectra.

With the help of the 3m-NIM (on the 3m-NIM-2 beamline), equipped with the 2 400 l/mm Pt-grating, we didn’t succeed to record any reliable photoabsorption spectrum over 1 eV photon energy range. This has been observed in the 5-25 eV region. Therefore, we swit-ched over to the 600 l/mm Fig.1 : Photoabsorption spectra in the 6-11 eV

photon energy range : (a) 1,1-difluoro- (b) 1,1-difluoro-2-chloro- and (c) 1,1- difluoro- 2-bromo-ethylenes.

6 7 8 9 10 11

0,0 0,2 0,4

Photon Energy (eV)

0,0 0,2

(c) BrHC=CF

2

log

10

[I

0

/I]

0,0 0,2

(a) H

2

C=CF

2

Photoabsorption Spectrum of

(b) ClHC=CF

2

(2)

Al-grating coated with a MgF2 layer. An important disadvantage of this type of grating is the presence of a reflectivity gap between 15-18 eV photon energy. Entrance and exit slit widths were adjusted at 25µm and 10µm respectively. Under these experimental conditions a resolution of 5000 is obtained.

careful investigations and further analysis for assignments.

Acknowledgment.

R.L. and B.L. gratefully acknowledge the Communauté Française de Belgique for the “Actions de Recherche Concertée” (A.R.C.) contract.

References.

[1]. F. Güthe, R. Locht, B. Leyh, H. Baumgärtel and K.M. Weitzel, J. Phys.Chem. 103 (1999) 8404. [2]. R. Locht, B. Leyh, K. Hottmann, and H. Baumgärtel, Chem.Phys. 220 (1997) 207. [3]. R. Locht, B. Leyh, K. Hottmann and H. Baumgärtel, Chem.Phys. 220 (1997) 217.

[4]. A. Hoxha, R. Locht, B. Leyh, D. Dehareng, K. Hottmann and H. Baumgärtel, Chem.Phys.

256 (2000) 239.

[5]. A. Hoxha, R. Locht, B. Leyh, D. Dehareng, K. Hottmann, H.W. Jochims and H. Baum-

gärtel, Chem.Phys. 260 (2000) 237.

[6]. A. Hoxha, R. Locht. A.J. Lorquet, J.C. Lorquet and B. Leyh, J. Chem.Phys. 111 (1999) 9259. [7]. G. Tornow, R. Locht, R. Kaufel, H. Baumgärtel and H.W. Jochims, Chem.Phys. 146

(1990) 115.

[8]. R. Locht, B. Leyh, K. Hottmann and H. Baumgärtel, BESSY Jahresbericht (1999) 150.

7,0 7,5 8,0 8,5 0,00 0,07 0,14 Photoaborption Spectrum of C2H3F between 6.7-8.6 eV log 10 [I0 /I]

Photon Energy (eV)

Fig.2 : Detail of the C2H3F photoabsorption spectrum between 6.7-8.6 eV photon energy.

Fig.1 shows typical photoabsorption spectra of 1,1-C2H2F2, 1,1-difluoro-2 chloro-and 1,1-difluoro-2-bromoethy-lene between 6-11 eV photon energy. In fact, spectra have all been recorded between 5-25 eV photon energy. The resolution achieved in the present experi-ment, as shown in fig.2, allows us to reconsider the Rydberg series assignments and to make a detailed vibrational analysis, in most cases, for the first time. Many spectra show extended vibrational structures, with long progressions, at high energies, i.e. above 12 eV excitation energy. These results require careful investigations and

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