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Electronic spectroscopy: Electronic transitions UV/VIS transitions - PowerPoint PPT Presentation

Electronic spectroscopy: Electronic transitions UV/VIS transitions between discrete electronic states. Electrons promoted from ground state to excited state. C---O e- excited e-C Oe- change bond order C---O vib ->


  1. Electronic spectroscopy:

  2. Electronic transitions UV/VIS transitions between discrete electronic states.  Electrons promoted from ground state to excited state.  C---O e- excited e-C — Oe- change bond order  C---O vib -> vibrate faster  C---O rot -> rotate faster  Rotational and vibrational transitions accompany  electronic transitions. Difficult to resolve all transitions  Molecular Spectroscopy CEM 484 2

  3. Energy level diagram Molecular Spectroscopy CEM 484 3

  4. Vibronic transitions Total energy need to include terms from al three transitions.  E total /hc = n ̃ elec + G( n ) + F(J)  E total /hc = n ̃ elec + ( n +1/2) n ̃ e – ( n +1/2) 2 x ̃ e n ̃ e + B ̃ n [J(J+1)] – D ̃ J 2 (J+1) 2  Rotational and vibrational terms are comparatively small and  not easily resolved. Ignoring rotations an expression for excitations between  excited state n ̃ obs = E 1, n ’ – E g, n ’’= 0 / hc = v ̃’ e1 + ( n ’+ 1/2) n ̃’ e – ( n ’+ 1/2) 2 x ̃’ e n ̃’ e - {v ̃’’ e0 +  n ̃’’ e /2 – x ̃’’ e n ̃’’ e /4 } Define: n 0,0 = ( n ̃ elec1 – n ̃ elec0 ) + n ̃’ e /2 – x' ̃ e n ̃’ e /4 – ( n ̃’’ e /2 – x ̃’’ e n ̃’’ e /4 )  n ̃ obs = n 0,0 + n ’ n ̃’ e – n ’( n ’+ 1)x ̃’ e n ̃’ e  Molecular Spectroscopy CEM 484 4

  5. Vibronic transitions Electronic energy  spectrum of I 2 . Higher energy  transitions become harder to resolve. Vibronic progression  Molecular Spectroscopy CEM 484 5

  6. Dissociation energy D o is dissociation energy.  Measured from the first vibrational state  Ground state is not at bottom of  potential well. D ̃ o = -E total /hc – D ̃ e – n ̃ e /2 + x ̃ e n ̃ e /4  Molecular Spectroscopy CEM 484 6

  7. Dissociation energies: Example The fundamental line in the infrared spectrum of 12 C 16 O  occurs at 2143.0 cm -1 , and the first overtone is found at 4260 cm -1 . Calculate the values of ν e and ν e x e for 12 C 16 O. Molecular Spectroscopy CEM 484 7

  8. Iclicker: Disociation energies The energy difference  4100 between two arbitrary 3900 levels n and n +1 is 3700 3500 D G (cm -1 ) D G = ṽ e (1 – 2x̃ e ( n + 1) )  3300 The dissociation energy  3100 y = -228.63x + 4154.7 R² = 0.9999 can be written as 2900 2700 D ̃ e = ṽ e (1-x ̃ e 2 )/4x ̃ e ≈  2500 ṽ e /4x ̃ e 0 1 2 3 4 5 6 7 v+1 Using the graph on  right, estimate the dissociation energy for H 2 . Molecular Spectroscopy CEM 484 8

  9. Electronic excitation intensity pattern Intensity pattern of electronic  transitions reveals molecular structure. Franck-Condon principle  Nuclei do not move appreciably during  electron excitation Molecular Spectroscopy CEM 484 9

  10. Iclicker: Label the curve Label the energy curve with:  Vibration and rotational quantum numbers.  The zero point energy for the ground electronic state.  The fundamental vibrational frequency of the ground electronic  state. The first overtone of the second electronic state.  The dissociation energy of the second electronic state.  The P-branch transition from the J=1, n =0 level in the ground  electronic state. The R-branch transition from the J=1, n =0 level in the ground  electronic state. Molecular Spectroscopy CEM 484 10

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