2010
DOI: 10.1016/j.jms.2010.06.010
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Laser excitation spectrum of C3 in the region 26000–30700cm−1

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Cited by 11 publications
(26 citation statements)
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“…Another unexpected result is that there is strong interaction between the overtones of the two stretching vibrations ν 1 and ν 3 . The interaction has matrix elements of the type <v a + 2, v b – 2| H | v a, v b >, characteristic of Darling–Dennison resonance .…”
Section: The ã State Of the C3 Radicalmentioning
confidence: 97%
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“…Another unexpected result is that there is strong interaction between the overtones of the two stretching vibrations ν 1 and ν 3 . The interaction has matrix elements of the type <v a + 2, v b – 2| H | v a, v b >, characteristic of Darling–Dennison resonance .…”
Section: The ã State Of the C3 Radicalmentioning
confidence: 97%
“…A thorough investigation of the vibrational structure of the trueA˜ state has been carried out using laser‐induced fluorescence from the products of the photolysis of allene under jet‐cooled conditions. Roughly 60 previously unidentified levels have been documented up to 30 700 cm −1 .…”
Section: The ã State Of the C3 Radicalmentioning
confidence: 99%
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“…23 C 3 is also the predominant carbon cluster in equilibrium hot carbon vapor, 19,24 hydrocarbon flames, 2,19 and plasmas generated through energetic processing of carbon containing materials. 19,25,26 The relevance of the C 3 molecule in space 27 as well as in terrestrial sooting flames and combustion processes 2,19 has motivated many experimental [28][29][30] and theoretical 17,18,[31][32][33][34][35][36][37][38][39][40][41] ) electronic manifolds. 23,[38][39][40] It is worth pointing out that, from the theoretical perspective, much effort has been devoted to obtain local (near-equilibrium) ground state potential energy surfaces 42 (PESs) for C 3 aiming to explore its spectroscopy, notably the unusual large amplitude bending motion and related speculations concerning its quasi-linearity (for a comprehensive review, see Refs.…”
Section: Introductionmentioning
confidence: 99%
“…Shi et al (2010) have obtained spectroscopic parameters in the isotopologues of CN through ab initio calculations. Moreover, experimental work on bands in the A 1 Π u − X 1 Σ + g system of C 3 has appeared (McCall et al 2003;Tanabashi et al 2005;Zhang et al 2005;Chen et al 2010Chen et al , 2011. Perturbations have been seen in many of these bands.…”
Section: Interstellar Mattermentioning
confidence: 99%