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1984
DOI: 10.1063/1.447453
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Direct absorption spectroscopy of jet-cooled polyenes. II. The 1 1B+u←1 1Ag transitions of butadienes and hexatrienes

Abstract: In the present paper, we report the direct absorption spectra of the 1 1B+u←1 1A−g transitions of gas phase butadiene, deuterated and methylated butadienes, and the cis and trans isomers of hexatriene cooled to low rotational and vibrational temperatures in supersonic molecular jets. These jet absorption spectra allow the more accurate determinations of Franck–Condon factors, upper state vibrational intervals and vibronic band homogeneous widths. We discuss the experimental constraints that the measurements re… Show more

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Cited by 158 publications
(72 citation statements)
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“…The excitation energy of the planar trans-hexa-1,3,5-triene calculated with TDDFT is in a fairly good agreement with the experimental datum 70 (see Table 4). Both density functionals employed, B3LYP and BH&HLYP, predict the excitation energies within 0.3 eV from the experimental figure.…”
Section: Scheme 2: Numbering Of Atoms In Trans-135-hexatrienesupporting
confidence: 72%
“…The excitation energy of the planar trans-hexa-1,3,5-triene calculated with TDDFT is in a fairly good agreement with the experimental datum 70 (see Table 4). Both density functionals employed, B3LYP and BH&HLYP, predict the excitation energies within 0.3 eV from the experimental figure.…”
Section: Scheme 2: Numbering Of Atoms In Trans-135-hexatrienesupporting
confidence: 72%
“…For the first four systems ͑up to five double bonds͒, the experimental transition energies in gas phase are known. [11][12][13][14][15][16][17][18][19] Table IV reports the experimental as well as the calculated vertical transition energies. Figure 3 shows the shift in the transition energies with respect to butadiene.…”
Section: Polyenesmentioning
confidence: 99%
“…Similarly, in Figure 1b the calculated and measured energy gaps between the 1A g and 1B u states are plotted with experimental values. 48 First comparing the SCI/FF and SDCI/SOS calculations, we see that the power-law fits for the two are nearly parallel for the calculations of R, with the SCI/FF results approximately a factor of 2 larger in all cases. We also observe stabilization of the ground-state energy relative to SCI when DCI is included.…”
mentioning
confidence: 99%