spectra.jpg (5257 bytes)


Molecular Spectroscopy


Data and Analysis:

Here are the two emission bands we observed; each has a P branch and an R branch.

To gather the emission spectrum of the laser, we used a thermocouple power gauge and a strip-chart recorder.  All data was taken with a potiential of 18,000 Volts across the plasma.  Due to the slow response time and the thermocouple, the emission peaks are smeared into one large emission mountain.   The top picture is the band corresponding to transitions from the (001) asymmetric vibrational mode to the (100) symmetric vibrational mode.  The left hump is the P branch and the right hump is the R branch.

wpe71.jpg (20876 bytes)

 

The next photo is the band corresponding to transitions from the (001) asymmetric vibrational mode to the (020) bending vibrational mode.  Again, we see the P branch on the left and the R branch on the right.  Although it is difficult to tell from the small photo, the separation of the peaks increases as we move farther from the band center (v0).

wpe72.jpg (23407 bytes)

 

Notice that in both bands, the P branch has a higher intensity than the R branch.  This results from a quantum mechanical effect whereby the wave functions overlap in such a way to make P branch transitions more probable than R branch transitions.   The following data was taken by hand-- it is the R branch of the transitions from (001) to (020).  We see that R(12) is right in the center of the maximum.

wpe3.jpg (8587 bytes)

    For the sake of time, we did not set up the equipment needed to measure the exact wavelengths corresponding to these molecular transitions. So, we use well known data to discuss the analysis of the emission spectrum as if we were able to know the exact values in our data.  According to Eastham, peaks in the first band have been observed from R(0) at 10.39 microns to R(62) at 10.02 microns as well as P(2) at 10.42 microns to P(68) at 11.18 microns.  The lasing transition with maximum intensity P(22) at about 10.6 microns (Eastham 205).  

    Knowing that the difference between rotational levels is , we can use a little algebra to calculate the E0 energy difference between the ground state (001) and the ground state of (100): E0= 1.91077 *10-20 J = 962.54 cm-1. For the rotational inertia, we calculate a value of:

I=9.766*10-39 g-cm2 (compare to HCL, for which I=2.60*10-40 g-cm2 (Shankland 153)).

 

The force constant and vibration frequency for the CO2 symmetric stretch mode can be calculated if we know the ground state energy for the symmetric stretch:

    E0 = 1388 cm-1   (Milonni 438)

, where mr is the reduced mass of the system

For the Symetric Stretch mode:

w = 5.226 * 1014 rad/s. This is about 83 trillion cycles per second, which is quite faster than most people can run.   For the H2 molecule, the frequency of vibration is even larger at  8.295*1014 rad/s (Sandin 254).

k = 3628.00 N/m. If a 200 pound person were to hang from a large metal spring with this same force constant, the spring would stretch about 25 cm.

Similar analysis may be performed with other diatomic and triatomic systems.    Molecular spectroscopy is a very useful tool to learn much about the interaction of molecules in a plasma.

 

Table of Contents:

  • Title Page

  • Molecular Spectroscopy and the CO2Molecule

  • Molecular Vibration Theory
    Data and Analysis

  • Multi-Photon Absorption in Cesium

  • Ionization Spectra
    Quantum Defect
    Cesium Energy Levels

  • Raman Spectroscopy: Four-Wave mixing in Sodium Atoms

  • Theory: Raman Scattering and Four-Wave Mixing
    Four Wave Mixing Data

  • Spectroscopic Aparatus

  • Page the First


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