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1994
DOI: 10.1016/0009-2614(94)00066-2
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Rotation of CN in solid rare gases

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Cited by 20 publications
(24 citation statements)
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“…The number results from line widths of the infrared emission spectrum that belongs to the X 2 state v = 1-3 transitions. Observations 21 of the weak Q branch due to a rotational barrier, and the related shift of the rotational constant (B e ≈ 1.6 cm −1 ) due to an induced Xe matrix inertia, are bypassed at the present account.…”
Section: Implementation Methodsmentioning
confidence: 86%
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“…The number results from line widths of the infrared emission spectrum that belongs to the X 2 state v = 1-3 transitions. Observations 21 of the weak Q branch due to a rotational barrier, and the related shift of the rotational constant (B e ≈ 1.6 cm −1 ) due to an induced Xe matrix inertia, are bypassed at the present account.…”
Section: Implementation Methodsmentioning
confidence: 86%
“…The rotational superposition appears purely as a phase evolution, where the relative timing among the packet depends on delay times. A decay of coherence can be introduced by multiplying the polarization P 21 have estimated a rotational relaxation rate of about 100 GHz for CN in solid Xe, which we shall use in Sec. III B.…”
Section: Implementation Methodsmentioning
confidence: 99%
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“…Very little is known about the orientational dynamics of molecules inside the rare gas matrices and analyzing this dynamics is the purpose of the present study. Small molecules ͑H 2 O, HCl, CN, and NH 3 ͒ may rotate essentially freely in certain rare gas matrices, 6,7 as seen from rovibrational sidebands in the IR spectrum. However, somewhat larger molecules of the size of, for example, CH 3 , rotate in a thermally activated, diffusive manner, a process that has been studied by electron paramagnetic resonance, [8][9][10] as well as by IR hole burning.…”
Section: Introductionmentioning
confidence: 99%