1986
DOI: 10.1103/physreva.34.1962
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Dipole moments and transition probabilities of thea3Σg+–b

Abstract: Multiconfiguration variational calculations are carried out of the electronic wave functions of the a X+ and b 3X+"states of molecular hydrogen, and the electric dipole transition moment between them is obtained. The dipole moment is used in a calculation of the probabilities of radiative transitions from the discrete vibrational levels of the a 'X~state to the vibrational continuum of the repulsive b 3X+ state as functions of the wavelength of the emitted photons, and a comparison is made with measurements of… Show more

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Cited by 23 publications
(15 citation statements)
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“…5 Therefore we have to analyze all available data about electron impact excitation and spontaneous decay of the upper levels.…”
Section: Constants Of Elementary Processesmentioning
confidence: 99%
See 1 more Smart Citation
“…5 Therefore we have to analyze all available data about electron impact excitation and spontaneous decay of the upper levels.…”
Section: Constants Of Elementary Processesmentioning
confidence: 99%
“…They were stimulated by molecular spectroscopy and quantum chemistry [1][2][3][4][5][6][7], investigations of hydrogen containing plasmas [8][9][10] and astrophysics [11,12]. Since the first work of Houtermans [13] the a 3 Σ + g → b 3 Σ + u transition has been studied as a possible laser system (see [14][15][16][17] and Refs.…”
Section: Introductionmentioning
confidence: 99%
“…The transition probability from a discrete vibrational state v to a continuum vibrational state with wavenumber k is calculated as [45][46][47]:…”
Section: Transition Presentmentioning
confidence: 99%
“…D(R) is the transition moment between the electronic states; ν vk is the frequency of the emitted light; and g is the statistical weight. Table 5 lists references for D(R) used in the present model, and ψ k (R) is calculated by applying the Numerov method [33] to Equation (7), and ψ k (R) is normalized at large R according to [46,47]. Table 5.…”
Section: Transition Presentmentioning
confidence: 99%
“…The a X i + b X: transition is also a major contributor to the opacity in stellar atmospheres [21]. The spectra resulting from electron-impact excitation of the a X i state of H2 and D2 have been measured and calculated with high accuracy [21].…”
mentioning
confidence: 99%