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Lecture 32 General issues of spectroscopies. II

Lecture 32 General issues of spectroscopies. II.

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Lecture 32 General issues of spectroscopies. II

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  1. Lecture 32General issues of spectroscopies. II (c) So Hirata, Department of Chemistry, University of Illinois at Urbana-Champaign. This material has been developed and made available online by work supported jointly by University of Illinois, the National Science Foundation under Grant CHE-1118616 (CAREER), and the Camille & Henry Dreyfus Foundation, Inc. through the Camille Dreyfus Teacher-Scholar program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the sponsoring agencies.

  2. General issues of spectroscopies • We will learn two types of spectroscopies: absorption/emission and scattering. • We will learn their relationship to dipole moment and polarizability as well as perturbation theories.

  3. Absorption/emission versus scattering spectroscopy • Absorption/emission spectroscopy: microwave, IR, and UV/vis absorption as well as fluorescence • Scattering spectroscopy: Raman IR Raman

  4. Absorption spectroscopy One-photon process 1st order perturbation theory

  5. Scattering (Raman) spectroscopy C. V. Raman Public domain image from Wikipedia Two-photon process 2nd order perturbation theory

  6. Scattering (Raman) spectroscopy Anti-Stokes Raman (a hot band) Stokes Raman Rayleigh

  7. Scattering (Raman) spectroscopy Resonant Rayleigh Resonant Raman Raman

  8. Quantum in nature Resonance Rayleigh scattering Why is sky blue?

  9. Quantum in nature Resonance Rayleigh scattering Why is the Sun yellow?

  10. Dipole moment and polarizability • Absorption spectroscopies (such as IR spectroscopy) are related to the dipole moment and its changes. • Scattering spectroscopies (such as Raman spectroscopy) are related to the polarizabilityand its changes. • Polarizability– softness of wave function; the larger the polarizability, the more easily the wave function is distorted by external electric field to create an induceddipole.

  11. Dipole moment + + + + + + + + + + + + Electric field Perturbation E0 E0 + µE – – – – – – – – – Think of molecular length! First-order perturbation theory

  12. Polarizability + + + + + + + + + + + + E0 + µE + αE2 =E0 + (µ+ αE)E E0 – – – – – – – – – Induced dipole Think of molecular volume! Second-order perturbation theory

  13. Polarizability + + + + + + + + + + + + – – – – – – – – –

  14. Classical (Smekal) theory of Rayleigh and Raman scattering • An oscillating electric field (incident photon) causes the molecule to have an induced dipole: • Polarizability varies with molecular vibration; so does induced dipole:

  15. Absorption/emission versus Raman spectroscopies • Absorption/emission occurs when molecular vibration, rotation, etc. alter dipole moment. The transition tends to transform as x, y, z. • Raman occurs when molecular vibration, rotation, etc. alter polarizability. The transition tends to transform as xx, yy, zz, xy, yz, zx.

  16. Summary • We have the general theories of absorption/emission spectroscopy and scattering (Raman) spectroscopy. • We have learned the relationship between absorption/emission spectroscopies to dipole moment and that between scattering (Raman) spectroscopy and polarizability. • We have made references to first- and second-order perturbation theories.

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