Module 3 : Molecular Spectroscopy
Lecture 13 : Rotational and Vibrational Spectroscopy
 

On either sides of the equilibrium bond length r0, the PE rises as a symmetric quadratic function (a parabola).  The vibrational wavefunctions can be obtained by solving the Schrodinger equation.  The Hamiltonian operator (for energy) now consists of a kinetic energy term and a potential energy term V as shown in Fig. 13.4 and the solutions for energy, Ev have already been given in Eq.(13.20).  The selection rules for the harmonic oscillator are:

Δv = ± 1                                                                                                                               (13.22)

We will see  several equally spaced lines (spacing hν) corresponding to the transitions 0→1, 1→2,  2→3 and so on.  The first transition will be the most intense as the state with v = 0 is the most populated.

In actual diatomics, the potential is anharmonic.  A good description of an anharmonic oscillator is given by the Morse function.

                                    P.E.  =  Deq [1 – exp {a(ro-r }]2                                                           (13.23)

In Eq. (13.22), Deq is the depth of the PE curve and r0 is the bond length.  A plot of the Morse curve and the energy levels for the Morse potential are given in Fig. 13.5.  The formula for the energy levels of this anharmonic oscillator is

                               

Ev/hc = ev  = (v+ ½) ν -  (v+ ½)2 ν xecm-1                                               (13.24)

Here xe, is called the anharmonicity constant whose value is near 0.01.  It can be easily deduced from the above formula that the vibrational energy levels for large υ start bunching together.

  Fig. 13. 5.   The Morse potential and the energy levels therein.  Note the difference between the dissociation energy Do and the depth Deq.  All molecules have a minimum of the zero point energy of hν/2 corresponding to the ν = 0 state.  This is a consequence of the uncertainty principle!