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Essentials of Computational Chemistry

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350 9 CHARGE DISTRIBUTION AND SPECTROSCOPIC PROPERTIES<br />

F<br />

F F<br />

I<br />

F<br />

∆<br />

I<br />

I<br />

hn<br />

F F<br />

+ I<br />

F<br />

F<br />

hn<br />

∆<br />

H<br />

H<br />

H H<br />

F<br />

F F<br />

retro-Bergman<br />

Bergman<br />

cyclization<br />

F<br />

+ I<br />

Figure 9.9 Bergman cycloaromatization reactions for hex-3-en-1,5-diyne and its perfluorinated<br />

congener, as well as a photochemical reaction scheme for generating the perfluorinated diradical<br />

from an iodinated precursor. What spectral features would be expected to be most diagnostic<br />

<strong>of</strong> the different intermediates? What levels <strong>of</strong> theory would be appropriate for predicting these<br />

spectral signatures? (Note that equilibrium arrows <strong>of</strong> unequal length indicate which species<br />

predominates at equilibrium.)<br />

Table 9.8 Experimental and computed IR spectra (cm −1 )forA,B,and<br />

C, and ITFP, PFPB, and PFHED, respectively<br />

A ITFP B PFPB C PFHED<br />

693 693 677 576<br />

834 834 690 591<br />

942/956 954 925 911 680<br />

1138 1145 1148 912 918<br />

1188 1195 1117 1151 1072 1067<br />

1259 1298 1154 1151<br />

1352 1400 1360 1363<br />

1428 1441 1407 1421 1398 1414<br />

1472 1487 1502/1516 1499 1678 1707<br />

1574 1585 1560 2337 2419<br />

1610 2426<br />

B3LYP/6-31G(d) in Table 9.3 would result in slightly improved agreement for A and C) as<br />

would be suggested by the synthetic scheme in Figure 9.9. Intensity data were also used,<br />

although those are not shown here; importantly, the ‘missing’ bands in the experimental IR<br />

spectra are all predicted to be <strong>of</strong> very low intensity in the computed spectra. Interestingly,<br />

both CASSCF and unrestricted B3LYP predict the singlet and triplet states <strong>of</strong> the diradical<br />

to be essentially degenerate, leaving the question open as to which (if either) is the lower<br />

in energy.<br />

hn<br />

H<br />

H<br />

F<br />

F<br />

H<br />

H<br />

F<br />

F

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