Electronic States and Band Spectrum Structure in Diatomic Molecules. VII. P2S2 and S2P2 Transitions

Robert S. Mulliken
Phys. Rev. 32, 388 – Published 1 September 1928
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Abstract

A survey is made of the varied empirical structure-types to be expected for P2S2 and S2P2 bands, and examples of these types are discussed individually. In agreement with Kemble's theory, the arrangement of the rotational levels in the P2 state changes continuously with the parameter ΔEB (ΔE=electronicdoubletseparation), and these changes are responsible for a large part of the observed variations in band structure. Fig. 1 and Table I show how the arrangement of the P2 levels changes with ΔEB, and Figs. 2-5 show, for the MgH, OH, HgH, and NO γ bands, how observed branches are related to energy levels. In Table II, data on ΔE and B are listed for a number of molecules. The mode of variation of the arrangement of the rotational levels in P2 states appears to be in striking agreement with the quantitative formulas of Hill and Van Vleck. For example, if ΔEB=+2, their equation becomes formally identical with the Kramers and Pauli formula which holds exactly for the P2 state of CH.

A consistent notation, as proposed in VI of this series, is given here for the known branches of the MgH, CaH, OH, ZnH, CdH, HgH, and NO bands; this notation has already been applied to the OH and BO bands (Kemble, Jenkins) and to CH λ3900. A more or less detailed discussion is given of the spectra mentioned, especially MgH and OH; some term values are given for P2 and S2 states of MgH, CaH and OH.

In the bands just mentioned, band-structure and missing lines show good agreement with theory. In the cases where |ΔEB| is small for the P2 state (CH, MgH) there is agreement with the case b intensity theory (six main branches, four weak satellite branches). As |ΔEB| increases, the satellite branches get stronger, and two new branches become evident. This tendency first appears distinctly in OH, where the satellite branches, although very weak, are much too strong for Hund's case b, and where a previously unclassified very weak branch is found to be one of the two new branches just mentioned. As |ΔEB| increases still further, the six weak branches finally become equal to the other six in intensity. This metamorphosis has also been discussed by Hulthén. The observed relations, in particular the equality of intensity of the six "weak" and the six "strong" branches when |ΔEB| is very large, appear to be in excellent agreement with the quantitative intensity formulas of Hill and Van Vleck.

A conclusion of interest for the empirical study of P2S2 and S2P2 bands is the following: in four-headed bands of these types the first head should always be weaker than the rest unless |ΔEB| is large, and should disappear if |ΔEB| is near zero.

Intensity relations in P3S3, P3S1, and other types of bands are briefly discussed for the case that one electronic state falls under Hund's case a, the other under his case b; some predictions are made.

  • Received 5 June 1928

DOI:https://doi.org/10.1103/PhysRev.32.388

©1928 American Physical Society

Authors & Affiliations

Robert S. Mulliken

  • Washington Square College, New York University

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Vol. 32, Iss. 3 — September 1928

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