Recommended conventions for defining transition moments and intensity factors in diatomic molecular spectra |
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Authors: | Ellis E. Whiting Aert Schadee Jeremy B. Tatum Jon T. Hougen Ralph W. Nicholls |
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Affiliation: | Ames Research Center, NASA, Moffett Field, California 94035 USA;“Sonnenborgh” Observatory, The Astronomical Institute at Utrecht, Zonnenburg 2, 3512 NL Utrecht, The Netherlands;University of Victoria, Victoria, British Columbia, Canada;National Bureau of Standards, Washington, D. C. 20234 USA;Center for Research in Experimental Space Science, York University, Downsview, Ontario, Canada |
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Abstract: | Two recommendations are made that can eliminate persistent confusion in the study of diatomic spectroscopy by providing uniform and consistent definitions of the electronic transition moments and the rotational line intensity factors. First, it is recommended that the equation for the line strength of a single rotational line be adopted to specify the relationship between the electronic transition moment and the rotational line intensity factor. Second, it is recommended that the electronic transition moment operator for perpendicular transitions be defined by (1/21/2)(μx ± iμy). The adoption of these conventions results in a value of (2S + 1)(2J + 1) for the sum rule of the rotational line intensity factor for Σ± ↔ Σ± transitions and a value of 2(2S + 1)(2J + 1) for the sum rule for all other spin-allowed transitions. |
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