1995
DOI: 10.1063/1.470376
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Vibrational population dynamics of the HgI photofragment in ethanol solution

Abstract: The vibrational population dynamics of HgI fragments in ethanol solution, resulting from the 320 nm photolysis of HgI 2 , are examined both experimentally and by a simulation. The experiments reveal an HgI population distribution which rapidly relaxes toward equilibrium. At the earliest times, the HgI exhibits vibrational coherent wave-packet motion that dephases with a time constant of ca. 1 ps. These data are used to gain insight into the character of the solvated potential energy curves. The population rela… Show more

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Cited by 78 publications
(68 citation statements)
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“…Agreement with the experiment is dependent upon the system or the calculation. In the case of mercury iodide, the calculated relaxation time, -2 ps, is in satisfactory agreement with the experiment, -3ps [62], whereas the agreement is poor for I; as stated above. However, the method presents qualitative analyses for the relaxation.…”
Section: B Classical Langevin Equationsupporting
confidence: 65%
“…Agreement with the experiment is dependent upon the system or the calculation. In the case of mercury iodide, the calculated relaxation time, -2 ps, is in satisfactory agreement with the experiment, -3ps [62], whereas the agreement is poor for I; as stated above. However, the method presents qualitative analyses for the relaxation.…”
Section: B Classical Langevin Equationsupporting
confidence: 65%
“…This has recently been studied by Pugliano et al [42]. This system forms a The next logical step would be to probe over a range of wavelengths in the visible region, especially further to the red.…”
Section: Vibrational Coolingmentioning
confidence: 99%
“…The formation of these bands is faster than our instrumental response time limited by solvent coherent artifact to about 400 fs. The 275-and 240-nm absorption bands are ascribed to a I·CH 3 CN charge-transfer complex (formation time in polar solvents, ≤ 0.3 ps, [4]) and a CH 2 Br· radical, [5], respectively. The absorption of CH 2 Br· and I·CH 3 CN shows no change up to 500 ps, suggesting that these species once formed following excitation of CH 2 BrI do not collapse within 500 ps to produce either the parent or the CH 2 Br-I isomer molecules.…”
mentioning
confidence: 99%