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Classical Theory of Raman Scattering
The classical theory of Raman effect, also called the polarizability theory, was developed by G. Placzek in 1934. I shall discuss it briefly here. It is known from electrostatics that the electric field 
where 
where 
Thus, from Eqs. (1) & (2),
Such an oscillating dipole emits radiation of its own oscillation with a frequency
where the coordinate q describes the molecular vibration. We can also write q as:
Where 
Substituting for
Making use of the trigonometric relation ![\sin x \sin y = \frac{1}{2} [\cos (x-y) -\cos (x+y) ]](http://s0.wp.com/latex.php?latex=%5Csin+x+%5Csin+y+%3D+%5Cfrac%7B1%7D%7B2%7D+%5B%5Ccos+%28x-y%29+-%5Ccos+%28x%2By%29+%5D+&bg=ffffff&fg=333333&s=0 "\sin x \sin y = \frac{1}{2} [\cos (x-y) -\cos (x+y) ]")
![\mu= \alpha_0 E_0 \sin 2\pi \nu t + \frac {1}{2} \frac {d\alpha}{dq} q_0 E_0 [\cos 2\pi (\nu - \nu_m) t - \cos 2\pi (\nu+\nu_m) t]](http://s0.wp.com/latex.php?latex=%5Cmu%3D+%5Calpha_0+E_0+%5Csin+2%5Cpi+%5Cnu+t+%2B+%5Cfrac+%7B1%7D%7B2%7D+%5Cfrac+%7Bd%5Calpha%7D%7Bdq%7D+q_0+E_0+%5B%5Ccos+2%5Cpi+%28%5Cnu+-+%5Cnu_m%29+t+-+%5Ccos+2%5Cpi+%28%5Cnu%2B%5Cnu_m%29+t%5D+&bg=ffffff&fg=333333&s=0 "\mu= \alpha_0 E_0 \sin 2\pi \nu t + \frac {1}{2} \frac {d\alpha}{dq} q_0 E_0 [\cos 2\pi (\nu - \nu_m) t - \cos 2\pi (\nu+\nu_m) t]")
Thus, we find that the oscillating dipole has three distinct frequency components:
1• The exciting frequency
2•
3•(2 & 3 with very small amplitudes of
. Hence, the Raman spectrum of a vibrating molecule consists of a relatively intense band at the incident frequency and two very weak bands at frequencies slightly above and below that of the intense band.
If, however, the molecular vibration does not change the polarizability of the molecule then 
Homonuclear diatomic molecules such as
which do not show IR Spectra since they don’t possess a permanent dipole moment, do show Raman spectra since their vibration is accompanied by a change in polarizability of the molecule. As a consequence of the change in polarizability, there occurs a change in the induced dipole moment at the vibrational frequency.
Related Articles
- Raman Effect- Raman Spectroscopy- Raman Scattering (wpgaurav.wordpress.com)
The Lindemann Theory of Unimolecular Reactions
It is easy to understand a bimolecular reaction on the basis of collision theory.
When two molecules A and B collide, their relative kinetic energy exceeds the threshold energy with the result that the collision results in the breaking of comes and the formation of new bonds.
But how can one account for a unimolecular reaction? If we assume that in such a reaction 
Raman Effect- Raman Spectroscopy- Raman Scattering
In constrast to other conventional brances of spectroscopy, Raman spectroscopy deals with the scattering of light & not with its absorption.
Raman Effect
- Raman Effect: An Overview
Chandrasekhar Venkat Raman discovered in 1928 that if light of a definite frequency is passed through any substance in gaseous, liquid or solid state, the light scattered at right angles contains radiations not only of the original frequency (Rayleigh Scattering) but also of some other frequencies which are generally lower but occasionally higher than the frequency of the incident light.
The phenomenon of scattering of light by a substance when the frequencies of radiations scattered at right angles are different (generally lower and only occasionally higher) from the frequency of the incident light, is known as Raman Scattering or Raman effect.
The lines of lower frequencies as known as Stokes lines while those of higher frequencies are called anti-stokes lines.
If f is the frequency of the incident light & f’ that of a particular line in the scattered spectrum, then the difference f-f’ is known as the Raman Frequency. This frequency is independent of the frequency of the incident light. It is constant and is characteristic of the substance exposed to the incident light.
A striking feature of Raman Scattering is that Raman Frequencies are identical, within the limits of experimental error, with those obtained from rotation-vibration (infrared) spectra of the substance.
Here is a home made video explaining the Raman Scattering of Yellow light:
And here is another video guide for Raman Scattering:
Advantage of Raman Effects
- Raman Spectroscopy can be used not only for gases but also for liquids & solids for which the infrared spectra are so diffuse as to be of little quantitative value.
- Raman Effect is exhibited not only by polar molecules but also by non-polar molecules such as O2, N2, Cl2 etc.
- The rotation-vibration changes in non-polar molecules can be observed only by Raman Spectroscopy.
- The most important advantage of Raman Spectra is that it involves measurement of frequencies of scattered radiations, which are only slightly different from the frequencies of incident radiations. Thus, by appropriate choice of the incident radiations, the scattered spectral lines are brought into a convenient region of the spectrum, generally in the visible region where they are easily observed. The measurement of the corresponding infrared spectra is much more difficult.
- It uses visible or ultraviolet radiation rather than infrared radiation.
Uses
- Investigation of biological systems such as the polypeptides and the proteins in aqueous solution.
- Determination of structures of molecules.
RAMAN was awarded the 1930 Physics Nobel Prize for this.
Classical Theory of Raman Effect
The classical theory of Raman effect, also called the polarizability theory, was developed by G. Placzek in 1934. I shall discuss it briefly here. It is known from electrostatics that the electric field
where
where
Thus, from Eqs. (1) & (2),
Such an oscillating dipole emits radiation of its own oscillation with a frequency
where the coordinate q describes the molecular vibration. We can also write q as:
Where
Substituting for
Making use of the trigonometric relation
Thus, we find that the oscillating dipole has three distinct frequency components:
1• The exciting frequency
2•
3•
If, however, the molecular vibration does not change the polarizability of the molecule then
Homonuclear diatomic molecules such as
REFERENCE:-
Principles in Physical Chemistry
[7th edition]
Puri, Sharma & Pathania
Dark Matter
A typical galaxy contains much more matter than what we can actually see. In fact, the visible portion of a galaxy represents only about 5 to 10% of total mass of the galaxy. Many studies lead us to define the conclusion that the Universe abounds in matter that we cannot see. This unseen matter is called Dark Matter because either it does not emit light or its light emission is too dim for us to detect.
Normal matter, such as STARS, PLANETS, DUST and MOLECULES , is often called Baryonic Matter because its mass is primarily due to the combined mass of the protons and neutrons, which are combinedly called Baryons, it contains. The mass of electrons is neglected because the mass of an electron is so small relative to the mass of a proton or neutron. Some of the normal matter such as burned out stars and dim interstellar gas, is part of the dark matter in a galaxy.
However, according to various calculations, this dark normal matter is only a small part of the total dark matter. The rest is called Non Baryonic Dark Matter because it does not contain proton and neutrons. What it contains? We know only one member of this type of dark matter…..the neutrinos.
