1974
DOI: 10.1063/1.1681797
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Mechanism for decay and spontaneous radiative decay constants of the lowest-lying attractive excited states of Ne2, Ar2, and Kr2

Abstract: Articles you may be interested inNonradiative decay of the lowest excited singlet state of 2-aminopyridine is considerably faster than the radiative decay

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Cited by 80 publications
(9 citation statements)
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“…A very slow tail in the solid has also been observed with a lifetime of 560 μs, attributed to excitations of the 3s 3 12 P 2 atomic state [8]; in one measurement of the liquid, an excited atomic triplet state was observed to decay nonexponentially, disappearing within several microseconds [43]. Measurements in gaseous neon suggest that long-lived 1 P 1 and 3 P 1 atomic states can react via three-body collisions to form radiative molecular states [45]; the lifetime of the long-lived molecular state in gas, presumably equivalent to the triplet state, was measured to be 6.6 μs [46]. Lastly, as the temperature of the gas is reduced, the emission due to molecular states disappears, leaving only the atomic spectra behind [8].…”
Section: A Time Dependence Discussionmentioning
confidence: 99%
“…A very slow tail in the solid has also been observed with a lifetime of 560 μs, attributed to excitations of the 3s 3 12 P 2 atomic state [8]; in one measurement of the liquid, an excited atomic triplet state was observed to decay nonexponentially, disappearing within several microseconds [43]. Measurements in gaseous neon suggest that long-lived 1 P 1 and 3 P 1 atomic states can react via three-body collisions to form radiative molecular states [45]; the lifetime of the long-lived molecular state in gas, presumably equivalent to the triplet state, was measured to be 6.6 μs [46]. Lastly, as the temperature of the gas is reduced, the emission due to molecular states disappears, leaving only the atomic spectra behind [8].…”
Section: A Time Dependence Discussionmentioning
confidence: 99%
“…Du point de vue th6orique, en dehors des estimations de Mulliken [11] illustr6es sur 1'exemple de Xe*, reprises par d'autres auteurs pour Ar* [12,13] et Kr* [14], seuls ont 6t6 publi6s a 1'heure actuelle les calculs d'lwata impliquant la configuration 2p' 3p du neon, ainsi qu'une etude preliminaire a vocation m6thodologique portant sur le croisement des 6tats g de Ar* corr6l6s aux configurations 3p' 4s et 3p' 4p par Teichteil et l'un des auteurs [15]. L'application directe de ces deux etudes concemait essentiellement 1'assignation des spectres d'absorption IR, motiv6e par les resultats exp6rimentaux de Oka et al [16,17]. En dehors des travaux precedents, les etudes spectroscopiques exp6rimentales restent parcellaires.…”
Section: Introductionunclassified
“…A theoretical value of 18 s for the lifetime of He 2 (a 3 Σ + u ) in the lowest vibrational state has been obtained by assuming the spin flip is driven by spin-orbit (SO) coupling and treating the Breit-Pauli spin-orbit Hamiltonian using first order perturbation theory [15]. The lifetimes of the lowest-energy triplet molecular states in neon, argon, krypton, and xenon are much shorter, measured to be 6.6 µs, 3.2 µs, 350 ns, and 50 ns respectively [16]. The large difference between the lifetimes of helium and the heavier noble gases is qualitatively due to the respective strengths of the SO coupling, which scales roughly as Z 4 .…”
mentioning
confidence: 99%