1992
DOI: 10.1063/1.462703
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Laser vaporization generation of B 14NH, B 15NH, B 14ND, B 16O, and B 17O: Electron-spin-resonance investigation in neon matrices under ultracold trapping conditions

Abstract: An investigation of collisional processes in a Dicke narrowed transition of water vapor in the 7.8 μ m spectral region by frequency down-chirped quantum cascade laser spectroscopy

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Cited by 40 publications
(27 citation statements)
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“…Knight et al 38,20 used this method to estimate the atomic orbital character of the singly occupied molecular orbital of BO, AlO, GaO, and InO. These FACM predictions reproduce the bonding trend that is shown in Table II for this series of metal oxide radicals: going from BO to InO the oxygen 2p character increases and the metal ns valence character decreases.…”
Section: A Electronic Structure Calculationsmentioning
confidence: 94%
“…Knight et al 38,20 used this method to estimate the atomic orbital character of the singly occupied molecular orbital of BO, AlO, GaO, and InO. These FACM predictions reproduce the bonding trend that is shown in Table II for this series of metal oxide radicals: going from BO to InO the oxygen 2p character increases and the metal ns valence character decreases.…”
Section: A Electronic Structure Calculationsmentioning
confidence: 94%
“…Values for the dipolar HFCCs at 5 bohr have been collected in Table 8 For GaO and its Rg complexes, HFCCs have been obtained only for Rg 12 and Rg 14 systems. They are displayed in Table 9 and will in the following section be used for comparison with the AlO and BO results.…”
Section: Resultsmentioning
confidence: 99%
“…A difference of about 20 MHz applied to the calculated gasphase value of 1466 MHz predicts an "experimental" gas-phase value of about 1445 MHz. The "experimental" A iso (Ga) in an Ar matrix is then estimated to be about 1890 MHz, arrived at by deducting 20 MHz from the value calculated for Ar 12 Hyperfine coupling constants can be related to the neutral and ionic structures I-III of the XO radicals, I being X(s 2 p 1 ) + O(s 2 p 4 ), II being X + (s 2 ) + O -(s 2 p 5 ), and III being X 2+ (s) + O 2-(s 2 p 6 ). Looking at the atomic open shells, A iso (X) is then due mainly to the doubly ionized structure III, which has an open-shell s orbital on X, and A dip (X) to the neutral structure I with an open p-shell on X.…”
Section: Discussionmentioning
confidence: 99%
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“…In 1992, the HNB was first observed by Knight et al [1] in their matrix electron spin resonance spectroscopy experiment. In 1995, Andrews and coworkers [2] reported the infrared spectroscopy experiment of HNB.…”
mentioning
confidence: 92%