VUV Spectroscopy of Atoms, Molecules and Surfaces
VUV Spectroscopy of Atoms, Molecules and Surfaces
VUV Spectroscopy of Atoms, Molecules and Surfaces
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4.5 CO − 2<br />
by sputtering, the situation is more unclear. Present in the decay are a<br />
number <strong>of</strong> not clearly resolvable lifetime components ranging from ∼100 µs<br />
to ∼100 ms, as shown in figure 4.4. The decay was only monitored out to<br />
140 ms due to a very low count rate for the ∼100 ms component. By fixing<br />
two <strong>of</strong> the components at 3.3 ms <strong>and</strong> 7.8 ms, the decay is fitted well with<br />
four exponentials <strong>and</strong> a (separately measured) constant background if data<br />
points corresponding to the first 400 µs are disregarded. For the remaining<br />
two components, values <strong>of</strong> 89 ms <strong>and</strong> 0.68 ms are thereby obtained. The neutral<br />
yield just after injection is underestimated by this fit, shown as the solid<br />
curve in figure 4.4. Since there is no reason for believing that the distribution<br />
over (vibrational) states should resemble that <strong>of</strong> the charge-exchange process,<br />
the data have also been fitted to three- <strong>and</strong> four freely varying exponentials,<br />
respectively. With three exponentials the very fast initial decay cannot be<br />
accounted for. Disregarding only the first 200 µs <strong>and</strong> fitting to four exponentials<br />
yields values for the the shortest- <strong>and</strong> longest-living components in<br />
the ranges 80–190 µs <strong>and</strong> 120–150 ms, respectively with the remaining two<br />
components ranging in the intervals 7.5–9.6 ms <strong>and</strong> 1.1–1.3 ms, respectively.<br />
The shortest-living component may indicate the presence <strong>of</strong> CO − 2<br />
73<br />
ions in<br />
the lowest-lying state, 2A1, <strong>and</strong> some <strong>of</strong> the millisecond components may be<br />
attributed to the unknown excited state(s) observed in the charge-exchange<br />
process. The ∼100 ms component representing ∼20% <strong>of</strong> the ions could be<br />
attributed to a very long-lived excited state <strong>of</strong> CO − 2<br />
not populated by the<br />
charge-exchange process. It could, however, also indicate contamination with<br />
a stable negative ion <strong>of</strong> mass 44 with a sufficiently low binding energy that it<br />
is sensitive to photodetachment by blackbody radiation. One possible c<strong>and</strong>idate<br />
is N2O − , for which a positive- as well as a negative adiabatic electron<br />
affinity have been suggested [47, 61]. Previous studies <strong>of</strong> the influence <strong>of</strong><br />
blackbody radiation on weakly-bound negative ions like Ca − ,Sr − <strong>and</strong> Ba −<br />
support this conclusion [62]. In spite <strong>of</strong> the possibility for contamination by<br />
the sputter process, it may be reasonable to assume that the CO − 2 ions observed<br />
by Middleton <strong>and</strong> Klein [10] are formed in the same electronic state(s)<br />
as the ones prepared by charge exchange <strong>and</strong> sputtering in the present investigation.<br />
The detection mode <strong>of</strong> the present experiment is, however, not<br />
mass-specific, so the monitored neutral yield could, in principle, be fragments<br />
. Assuming that pre-dissociation sets<br />
generated by pre-dissociation <strong>of</strong> CO − 2<br />
the lower limit on the lifetime, the CO − 2 statemustbeevenmorestablewith<br />
respect to autodetachment.