1997
DOI: 10.1063/1.475175
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Jet spectroscopy, structure, anomalous fluorescence, and molecular quantum beats of silylidene (H2C=Si), the simplest unsaturated silylene

Abstract: Articles you may be interested inElectronic spectroscopy of jet-cooled H C P + : Molecular structure, phosphorus hyperfine structure, and Renner-Teller analysis Polarization quantum beat spectroscopy of HCF (Ã 1 A ″ ). II. Renner-Teller and spin-orbit mixing in the simplest singlet carbeneThe electronic spectrum, molecular structure, and oscillatory fluorescence decay of jet-cooled germylidene ( H 2 C= 74 Ge ), the simplest unsaturated germylene

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Cited by 50 publications
(25 citation statements)
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References 48 publications
(43 reference statements)
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“…Although silicon analogs of many pure carbon clusters (C n ) and acetylenic free radicals (C n H) have recently been characterized by high-resolution spectroscopy (1,2), only H 2 CSi, the silicon analog of vinylidene (H 2 CC:), has been reported in the gas phase (3,4). Because small silicon-bearing molecules such as SiS, SiC, and SiC 2 , and the cumulene carbenes H 2 C 3 (5), H 2 C 4 (6), and H 2 C 6 (7) are abundant in the circumstellar shells of evolved carbon stars (8), H 2 CCSi and longer silacumulenes are plausible candidates for astronomical detection.…”
Section: Introductionmentioning
confidence: 99%
“…Although silicon analogs of many pure carbon clusters (C n ) and acetylenic free radicals (C n H) have recently been characterized by high-resolution spectroscopy (1,2), only H 2 CSi, the silicon analog of vinylidene (H 2 CC:), has been reported in the gas phase (3,4). Because small silicon-bearing molecules such as SiS, SiC, and SiC 2 , and the cumulene carbenes H 2 C 3 (5), H 2 C 4 (6), and H 2 C 6 (7) are abundant in the circumstellar shells of evolved carbon stars (8), H 2 CCSi and longer silacumulenes are plausible candidates for astronomical detection.…”
Section: Introductionmentioning
confidence: 99%
“…Table III gives the predicted excitation energies obtained in this work, and compares the 1 B 2 -1 A 1 excitation energy with the experimental T 0 . 19 The agreement is excellent; our best method, CISDϩQ TZ(2d f ,2pd), differs from experiment by only 0.2 kcal/mol. Notice, too, that the singlet and triplet A 2 states differ in energy by only 3 kcal/mol, while the singlet and triplet B 2 states differ in energy by 28 kcal/ mol.…”
Section: Resultsmentioning
confidence: 83%
“…This frequency is anomalously low, ϳ265 cm Ϫ1 , in the ground state, 13,17 and increases to 731 cm Ϫ1 in the 1 B 2 state. 19 Our theoretical predictions are 327 cm Ϫ1 in the ground state, and 795 cm Ϫ1 in the excited state. Thus, theory is about 60 cm Ϫ1 above the experimental value for each state.…”
Section: Resultsmentioning
confidence: 97%
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“…Well-known examples of molecules that exhibit anomalous fluorescence in violation of Kasha's rule include azulene and several of the thiocarbonyl compounds ͑XYC= S͒. 34 More recently, we have discovered 35,36 that H 2 C = Si and H 2 CGe also fluoresce from the B 1 B 2 excited state, with a variety of interesting photophysical properties, including single rotational level fluorescence decays that exhibit molecular quantum beats. The occurrence of anomalous emission from all these molecules is attributable to their unique energy level structure in which the second excited electronic state is far removed from the first, so that coupling between the two excited states is minimal.…”
Section: Excited State Photophysicsmentioning
confidence: 98%