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August 18, 2010 11:37      9in x 6in     b985-ch11     Elementary Physical Chemistry















                                                     Chapter 11

                                  Elements of Molecular Spectroscopy








                            11.1. Vibration–Rotation Spectra of Diatomic Molecules

                            Two points should be emphasized:
                             1. Actual energy levels are not directly measurable.
                             2. A spectrum shows only transitions of energy.


                            11.2. Rotational Selection Rules
                            Spectral absorption or emission corresponds to transitions between pairs
                            of levels, as noted before. But not all possible levels may be combined.
                            By theoretical studies of the wave-functions, especially their symmetry
                            properties, one can devise selection rules. These rules tell whether certain
                            quantum jumps are allowed or not allowed. Selection rules do not tell
                            whether the intensities are weak or strong.
                               The rotational energy levels of a linear molecule are
                                                            2
                                          E J = J(J +1)(h/2π) /2I  J =0, 1, 2,...      (11.1)
                            where J is the rotational quantum number, and I is the moment of inertia,
                                        2
                            namely I = µd (d being the internuclear distance and µ the reduced mass).
                            The results are generally expressed in terms of the rotational constant, B,
                            which has the dimensions of Hz (s −1 ) and is defined as
                                                               2
                                                      B =(h/8π I)                     (11.2a)
                            or, in terms of B , defined as
                                          ∗
                                                        B = B/c                       (11.2b)
                                                         ∗
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