4-2 SCATTERING BY AN ELECTRON
We have seen in chapter 1 that an x-ray beam is an electromagnetic wave characterized by an electric field whose strength varies sinusoidally with time at any one point in the beam. Since an electric field exerts a force on  a charged particle such as an electron, the oscillating electric field of an x-ray beam will set any electron it encounters into oscillatory motion about its mean position.
Now an accelerating or decelerating electron emits an electromagnetic wave. We have already seen an example of this phenomenon in the x-ray tube, where x-ray are emitted because of the rapid deceleration of the electrons striking the target. Similarly, an electron which has been set into oscillation by an x-ray beam is continuously accelerating and decelerating during its motion and therefore  emits an electromagnetic wave. In this sense, an electron is said to scatter x-rays, the scattered beam being simply the beam radiated by the electron under the action of the incident beam. The scattered beam has the same wavelength and frequency as the incident beam and is said to be coherent with it, since there is a definite relationship between the phase of the scattered beam and that of the incident beam which produced it. (the phase change on scattering from an electron is λ/2. Because it is exactly the same for all the electrons in a crystal, it cancels out in any consideration of phase differences between rays scattered by different atoms, as in fig. 3-2, and so does not affect the derivation of the Bragg law given in Sec. 3-2).
Although x-ray are scattered in all directions by an electron, the intensity of the scattered beam depends on the angle of scattering, in a way which was first worked out by J. J. Thomson. He found that the intensity I of the beam scattered by a single electro of charge e coulombs (C) and mass m kg, at a distance r meters from the electron, is given by

Where Io = intensity of the incident beam, μo= 4π x 10-7 m.kg.C-1, K= constant, and α= angle between the scattering direction and the direction of acceleration of the electron.


        
           Fig. 4-3
Suppose the incident beam is travelling in the direction Ox (Fig. 4-3) and encounters an electron  at O. we wish to know the scattered intensity at P in the xz plane where OP is inclined at a scattering angle of 2θ to the incident beam. An unpolarized incident beam, such as that issuing from an x-ray tube, has its electric vector E in a random direction in the yz plane. Ths beam may be resolved into two plane-polarized components, having electric vectors Ey and Ez where



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The y component of the incident beam accelerate; the electron in the direction Oy. It therefore gives rise to a scattered beam whose intensity at P is found from Eq. (4-1) to be
                       

Since α = ΔyOP = π/2. Similarly, the intensity of the scattered z component is given by
              
         
Since α = π/2 - 2θ. The total scattered intensity at P is obtained by summing the intensities of these two scattered components:
                                                                            
This is the Thomson equation for the scattering of an x-ray beam by a single electron. The intensity of the scattered beam is only a minute fraction of the intensity of the incident beam; the value of K is 7,94 x 10-30 m2, so that Ip/Io is only 7,94 x 10-26 in the forward direction at 1 cm from the electron. The equation also shows that the scattered intensity decreases as the inverse square of the distance from the scattering electron, as one would expect, and that the scattered beam is stronger in forward or backward directions than in a direction at right angles to the incident beam.
The Thomson equation gives the absolute intensity (in ergs/sq cm/sec) of the scattered beam in terms of the absolute intensity of the incident beam. These absolute intensities are both difficult to measure and difficult to calculate, so it is fortunate that relative values are sufficient for our purposes in practically all diffraction problems. In most cases, all factors in Eq. (4-2) except the last are constant during the experiment and can be omitted. This last factor, 1/2 (1+cos22θ), is called the polarization factor; this is a rather unfortunate term because, as we have just seen, this factor enters the equation simply because the incident beam is unpolarized. The polarization factor is common to all intensity calculations, and we will use it later in our equation for the intensity of a beam diffracted by a crystalline powder.
There is another and quite different way in which an electron can scatter x-rays, and that is manifested in the Compton effect. This effect, discovered by A. H. Compton in 1923, occurs whenever x-rays encounter loosely bound or free electrons and can be understood only by considering the incident beam not as a wave motion, but as a stream of x-ray quanta or photons, each of energy hv1. When such a photon strikes a loosely bound electron, the collision is an elastic one like that of two billiard balls (Fig. 4-4). The electron is knocked aside and the photon is deviated through an angle 2θ. Since some of the energy of the incident photon is used in providing kinetic energy for the electron, the energy hv2 of the photon after impact is less than its energy hv1 before impact. The wavelength λ2 of the scattered radiation is thus slightly greater than the wavelength λ1 of the incident beam, the magnitude of the change being given by the equation
                                                     
                       (4-3)
The increase in wavelength depends only on the scattering angle, and it varies from zero in the forward direction (2θ = 0) to 0.05 Ǻ in the extreme backward direction (2θ = 180).
Radiation so scattered is called Compton modified radiation, and, besides having its wavelength increased, it has the important characteristic that its phase has no fixed relation to the phase of the incident beam. For this reason it is also known as incoherent radiation. It cannot take part in diffraction because its phase is only randomly related to that of the incident beam and cannot therefore produce any interference effects. Compton modified scattering cannot be prevented, however, and it has the undesirable effect of darkening the background of diffraction patterns.
(it should be noted that the quantum theory can account for both the coherent and the incoherent scattering, where as the wave theory is applicable only to the former. In terms of the quantum theory, coherent scattering occurs when an incident photon bounces off an electron which is so tightly bound that the electron receives no momentum from the impact. The scattered photon therefore has the same energy, and hence wavelength, as it had before).



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