2001
DOI: 10.1006/jmsp.2001.8459
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IR Spectrum of C8H2: Integrated Band Intensities and Some Observational Implications

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Cited by 35 publications
(35 citation statements)
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“…The chemical shifts computed with the CAM-B3LYP functional compare well with earlier experimental and computed values reported for PY chains [35][36][37][38] . For PY with n=16, the chemical shift we predict ranges between 56-65 ppm, which compares very well to the experimental value reported by Tykwinski (57-69 ppm) 38 .…”
Section: Methodssupporting
confidence: 80%
“…The chemical shifts computed with the CAM-B3LYP functional compare well with earlier experimental and computed values reported for PY chains [35][36][37][38] . For PY with n=16, the chemical shift we predict ranges between 56-65 ppm, which compares very well to the experimental value reported by Tykwinski (57-69 ppm) 38 .…”
Section: Methodssupporting
confidence: 80%
“…H(-C≡C-) m H, H(-C≡C) m or (C≡C) m ). Khlifi et al (1995); (i) Shindo et al (2001Shindo et al ( , 2003. Comparing our UV-VIS spectra to spectra obtained by arcing of graphitic electrodes submerged in water (Cataldo 2004), also shown in Fig.…”
Section: Polymerizationmentioning
confidence: 64%
“…The aforementioned reaction products have known vibrational transitions both in the short wavelength range of the C-H stretching mode and around the C-H bending mode. Shindo et al (2001Shindo et al ( , 2003 and A83, page 4 of 11 Zhou et al (2009) have observed other stronger features at 600, ∼620, 664, ∼3330, and 3386 cm −1 . Owing to a combination of the water baseline and worsened signal-to-noise ratios in these parts of the spectrum, these features are not unambiguously identified in our spectra.…”
Section: Polymerizationmentioning
confidence: 98%
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“…Finally, investigations of the atmosphere of Titan, a moon of Saturn, have shown that photochemistry in its upper atmosphere leads to significant concentrations of polyynes, assumed to be produced in similar reaction sequences to those involved in the terrestrial formation of PAHs and soot, and including ethynyl-like intermediates in a chain reaction synthetic pathway. [12][13][14] In support of the extensive reaction network modeling in multiple environments, rate constants have been measured for reactions of ethynyl radicals with various partners over a range of temperatures. [15][16][17][18][19][20][21][22][23][24][25] Following the astronomical observation of the ethynyl radical, 9 the gas-phase microwave spectrum was recorded and the molecular structure determined in the 1980's.…”
Section: Introductionmentioning
confidence: 99%