Phys. Chem. Chem. Phys., 1999, 5121

Additions and corrections

The S0S1 cavity ring-down absorption spectrum of jet-cooled azulene: dependence of internal conversion on the excess energy

A. A. Ruth, E.-K. Kim and A. Hese

Phys. Chem. Chem. Phys., 1, 5121. (DOI: 10.1039/a906344g) . Amendment published on the Web 21st July 2000

The authors wish to apologise for an unfortunate but severe mistake in the above publication in the evaluation of the homogeneous linewidths. Instead of the full width at half maximum the half width at half maximum was used for the Lorentzian lineshape in the published evaluation procedure. The correct homogeneous linewidth for the S0,0S1,0 transition of jet-cooled azulene reported by us to be 2.0 + 0.25 cm–1 (in the text and also in Fig. 3a) should therefore be 4.0 + 0.5 cm–1 corresponding to an S1,0 lifetime of (S1)= 1.30 ps with error limits of +0.22 and –0.12 ps. Consequently all values for hom of vibronic transitions S0,0S1,v in the fifth column of Table 1 should also be larger by a factor of 2. This mistake affects the two sections on the comparison with published S1 lifetimes in the discussion: Our previous conclusion that the molecular environment does not significantly perturb the azulene dynamics must be revised; although our measurement yields a slightly larger value for (S1.0) of jet-cooled azulene than previously reported S1,0 lifetimes (0.8 + 0.2,1 1.1 + 0.2,2 1.1 3 ps), this result corroborates1 a significant medium effect on the intramolecular relaxation of the S1 electronic origin when compared to measurements in solid matrix [(S1,0)~ 2.6 or 3.3 ps]4,5 at low temperatures or with time domain measurements in solution (1.0,6 1.7 ps 7). Shorter decay times in the isolated molecule still exist at an excess energy of 2000 cm–1 where our value for the IC decay time is now ~0.5 ps in comparison to time domain measurements yielding 0.9 ps in the jet.8

Finally, statements in the Introduction should be read with caution and the corrected value for the S1,0 lifetime in mind!

We would like to genuinely apologise for this error and would like to thank Dr C. Cossart-Magos and Prof. J. Jortner sincerely for bringing this flaw to our attention.

References

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4 R. M. Hochstrasser and T.-Y. Li, J. Mol. Spectrosc., 1972, 41, 297.
5 R. M. Hochstrasser and C. A. Nyi, J. Chem. Phys., 1979, 70, 1112.
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8 E. W.-G. Diau, S. DeFeyter and A. H. Zewail, J. Chem. Phys., 1999, 110, 9785.


The Royal Society of Chemistry apologises for these errors and any consequent inconvenience to authors and readers.


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