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Dissociative electron attachment to the unstable carbon ...

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<strong>Dissociative</strong> <strong>electron</strong> <strong>attachment</strong> <strong>to</strong> CS 7<br />

Counts<br />

18000<br />

16000<br />

14000<br />

12000<br />

10000<br />

8000<br />

6000<br />

4000<br />

2000<br />

0<br />

(a)<br />

CS +<br />

CS 2<br />

+<br />

10 12 14 16 18 20<br />

Electron Energy (eV)<br />

Counts<br />

25000<br />

20000<br />

15000<br />

10000<br />

5000<br />

0<br />

(b)<br />

CS +<br />

CS 2<br />

+<br />

10 12 14 16 18 20<br />

Electron Energy (eV)<br />

Figure 7. Intensities of CS + and CS + 2 observed with (a) <strong>the</strong> plasma off and (b) <strong>the</strong><br />

plasma on as a function of <strong>electron</strong> energy. The presence of CS in <strong>the</strong> gas sample with<br />

<strong>the</strong> plasma on is confirmed by <strong>the</strong> appearance of CS + at <strong>the</strong> ionization energy of CS.<br />

Counts<br />

600<br />

500<br />

400<br />

300<br />

200<br />

100<br />

0<br />

(a)<br />

C 2 S +<br />

C 3 S 2<br />

+<br />

10 12 14 16 18 20<br />

Electron Energy (eV)<br />

Counts<br />

400<br />

350<br />

300<br />

250<br />

200<br />

150<br />

100<br />

50<br />

0<br />

(b)<br />

S 2 O +<br />

SO +<br />

10 12 14 16 18 20<br />

Electron Energy (eV)<br />

Figure 8. (a) Intensities of C 2 S + and C 3 S + 2 as a function of <strong>electron</strong> energy with <strong>the</strong><br />

plasma on at high CS 2 inlet pressure and (b) intensities of SO + and S 2 O + with <strong>the</strong><br />

plasma on with low CS 2 inlet pressure.<br />

energy of CS + from CS 2 .<br />

CS is known <strong>to</strong> undergo spontaneous polymerisation reactions leading <strong>to</strong> species of<br />

<strong>the</strong> type C n S m . Proposed reactions leading <strong>to</strong> <strong>the</strong> formation of C 3 S 2 are [26]<br />

2CS → C 2 S + S (2)<br />

C 2 S + CS → C 3 S 2 (3)<br />

C 3 S + 2 and also weakly C 2 S + were observed in <strong>the</strong> positive ion mass spectrum with <strong>the</strong><br />

plasma on. Most of <strong>the</strong> C 2 S + detected, however, is likely <strong>to</strong> be due <strong>to</strong> dissociation of a<br />

larger ion ra<strong>the</strong>r than ionization of C 2 S as <strong>the</strong> observed appearance energy is relatively<br />

high at 15.5 ± 0.5 eV, see Figure 8(a). The ionization threshold of C 3 S 2 is determined<br />

<strong>to</strong> be 9.4 ± 0.3 eV from <strong>the</strong> data shown in Figure 8(a). This is in good agreement<br />

with a predicted vertical ionization energy of 9.19 eV calculated here with a GAMESS

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