1994
DOI: 10.1103/physreva.50.2304
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Rotational and vibrational lifetime of isotopically asymmetrized homonuclear diatomic molecular ions

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Cited by 77 publications
(55 citation statements)
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“…The cooling rate and the resulting population distribution finally reached are determined by the interaction with the blackbody radiation field of 300 K that pervades the inner volume of the room-temperature ion storage ring, and by the continuous interaction of the HD + ions with the electrons of the electron cooler and the electron target. While the Einstein coefficients between the rotational states required to describe the interaction of HD + with the radiation field are well known [35], the expected large inelastic cross sections for low-energetic electron scattering on rotational states of HD + could only recently be verified by observing the rotational cooling of HD + by super-elastic electron collisions (SEC) in a dedicated experiment [23]. Based on these findings we estimated the time development of the rotational populations by adjusting the calculations described by Shafir et al [23] to the present experimental situation.…”
Section: Resultsmentioning
confidence: 99%
“…The cooling rate and the resulting population distribution finally reached are determined by the interaction with the blackbody radiation field of 300 K that pervades the inner volume of the room-temperature ion storage ring, and by the continuous interaction of the HD + ions with the electrons of the electron cooler and the electron target. While the Einstein coefficients between the rotational states required to describe the interaction of HD + with the radiation field are well known [35], the expected large inelastic cross sections for low-energetic electron scattering on rotational states of HD + could only recently be verified by observing the rotational cooling of HD + by super-elastic electron collisions (SEC) in a dedicated experiment [23]. Based on these findings we estimated the time development of the rotational populations by adjusting the calculations described by Shafir et al [23] to the present experimental situation.…”
Section: Resultsmentioning
confidence: 99%
“…Based on the potential energy curve [20] f ) for rovibrational transitions connecting initial (i) and final (f ) rovibrational levels; the same approach and approximations as in Ref. [44] were used [45]. Since the spin-rotational interaction is negligible, the rotational quantum numbers are J = 0, 1, 2, .…”
Section: Radiative Thermalizationmentioning
confidence: 99%
“…The closed set of energy levels coupled by the two-photon spectroscopy scheme is shown in Figure 2. The rovibrational levels have small radiative decay widths, for example Γ 3 /(2Ï€) = 0.037 Hz and Γ 5 /(2Ï€) = 13.1 Hz [28]. …”
Section: Two-photon Spectroscopy Schemementioning
confidence: 99%
“…The closed set of energy levels coupled by the two-photon spectroscopy scheme is shown in Figure 2. The rovibrational levels have small radiative decay widths, for example Γ3/(2Ï€) = 0.037 Hz and Γ5/(2Ï€) = 13.1 Hz [28]. The parameters used for modelisation are taken from the experimental setups with HD + ions (see for example [17]).…”
Section: Two-photon Spectroscopy Schemementioning
confidence: 99%