THE INFRARED SPECTRA AND THE MOLECULAR STRUCTURE OF PYRAMIDAL $MOLECULES^{\ast}$

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1952

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Ohio State University

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The two nearly coincident vibration frequencies ω1 and ω3 and the overlapping bands ω2 and ω4 (Herzberg's notation) of XH3 molecules are coupled, respectively, by Coriolis interactions. It is possible to show that in the case of ω1 and ω3 the interaction is so slight that it may satisfactorily be taken into account in the effective moments of inertia.1 Standard methods, using combination relations, may therefore be employed in the analysis of these bands. The Coriolis coupling between ω2 and ω4 is not small, however, and the interaction must be calculated by the use of degenerate perturbation methods.2 It may be shown, however, that for values of the quantum number K=J and K=JI (i.e., where the rotation of the molecule classically is almost entirely about the axis of symmetry) the perturbation is small enough so that the corresponding term values in the first excited state of ω4 may be obtained by an expansion of the secular determinant. One may show by this method that the frequency interval between two RR lines, RR(J,K) and RR(J+1,K+1) is equal to Δν=2[(1−ζ4)C+2ζ2.42B2/Δ] where B=h/8πIxxc and C=h/8π2Izzc,Ixx and Izz being the two moments of inertia, ζ4 is the degenerate Coriolis coefficient coupling the incipient angular momentum of ω3 and ω4 to the rotation of the molecule and where Δ=ω4ω3. Similarly one may show that the frequency interval between two RR lines RR(J,K−1) and RR(J+1,K) is equal to Δv′=2[(1−ζ4)C−4ζ2.42B2/Δ]. A direct means of determining the magnitude of the perturbation from the experimental data is therefore available if the above lines can be identified. The term values of ω3 where K=O (i.e., where the molecule is tumbling) may also readily be obtained from the secular determinant. Here also the frequency interval between two lines in the P branch were K=O gives a measure of ζ2.42B2/Δ. When applied to the molecules PH3,3AsH3, and SbH3 and recalling that ζ2+ζ4=(B/2C)−1 the following values for the H-X-H angle, α, and the XH distance r, are obtained: for PH3,α=9350′,r=1.424 {\AA}; for Ash3,α=9135′,r=1.523 {\AA}; and for SbH3,α=9130′,r=1.711 {\AA}. These values agree within experimental error with the values given by Loomis and Strandberg4 from microwave data.

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Author Institution: Department of Physics and Astronomy, The Ohio State University,

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