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Lecture 32 Lecture 32

Lecture 32 - PowerPoint Presentation

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Lecture 32 - PPT Presentation

General issues of spectroscopies II c So Hirata Department of Chemistry University of Illinois at UrbanaChampaign This material has been developed and made available online by work supported jointly by University of Illinois the National Science Foundation under Grant CHE1118616 CARE ID: 265735

spectroscopy raman dipole scattering raman spectroscopy scattering dipole absorption polarizability emission spectroscopies perturbation moment theory molecular order rayleigh induced

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Slide1

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

.Slide2

General issues of spectroscopiesWe 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.Slide3

Absorption/emission versus scattering

spectroscopy

Absorption/emission spectroscopy

: microwave, IR, and UV/

vis

absorption as well as fluorescence

Scattering spectroscopy

: Raman

IR

RamanSlide4

Absorption spectroscopy

One-photon process

1

st

order perturbation theorySlide5

Scattering (Raman) spectroscopy

Two-photon process

2

nd

order perturbation theory

C. V. Raman

Public domain image from WikipediaSlide6

Scattering (Raman) spectroscopy

Rayleigh

Anti-Stokes

Raman

(a hot band)

Stokes

RamanSlide7

Scattering (Raman) spectroscopy

Resonant

Rayleigh

Resonant

Raman

RamanSlide8

Quantum in nature

Why is sky blue?

Resonance Rayleigh scatteringSlide9

Quantum in nature

Why is the Sun yellow?

Resonance Rayleigh scatteringSlide10

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 polarizability

and 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 induced dipole.Slide11

Dipole moment

E

0

E

0

+

µE

+ + + + + + + + + + + +

– – – – – – – –

First-order perturbation theory

Electric field

Perturbation

Think of

molecular

length!Slide12

Polarizability

E

0

E

0

+

µE +

α

E

2

=

E

0 + (µ

+ αE)E

+ + + + + + + + + + + +

– – – – – – – –

Second-order perturbation theory

Induced dipole

Think of

molecular

volume!Slide13

Polarizability

+ + + + + + + + + + + +

– – – – – – – – Slide14

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: Slide15

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

.Slide16

SummaryWe 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.