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PHYS01200804001 Sohrab Abbas - Homi Bhabha National Institute

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2.2.3.2 Symmetric Laue case<br />

For an infinite incident plane wave, the α and β wave functions combine at the exit surface in<br />

accordance with the boundary conditions to generate a forward transmitted and a diffracted wave in<br />

vacuum. In order to simplify the relevant expressions without losing generality, we restrict<br />

ourselves to the symmetric Laue case in a parallel-faced crystal slab and a full reflection (χ O = χ H ).<br />

The amplitudes of the emergent waves can then be written as<br />

it(1<br />

y)<br />

<br />

V <br />

t S<br />

2<br />

y t<br />

2<br />

<br />

T(y, t) O<br />

(y, t) e cos y 1 i sin y 1<br />

<br />

<br />

2<br />

S<br />

y 1<br />

<br />

S<br />

<br />

(38a)<br />

and<br />

R(y, t) (y, t) ie<br />

V<br />

H<br />

<br />

i t(1 y) 2Zf<br />

y<br />

S<br />

<br />

<br />

<br />

<br />

<br />

<br />

<br />

t<br />

<br />

S<br />

2<br />

sin y 1<br />

2<br />

y 1<br />

<br />

<br />

<br />

<br />

<br />

<br />

, (38b)<br />

t denoting the slab thickness and Z f being the distance of the incidence surface from the origin<br />

measured along n i . As explained in Fig.5, the ψ O , wave emanates exactly along the incidence<br />

direction, represented by y, whereas the ψ H wave exits at an angle corresponding to -y with the<br />

exact Bragg condition. The associated intensities<br />

I (y, t) 1 I (y, t) , (39a)<br />

O<br />

H<br />

with<br />

I (y, t) <br />

t<br />

<br />

<br />

y 1<br />

2 2<br />

sin y 1<br />

S<br />

H 2<br />

<br />

<br />

<br />

; (39b)<br />

are both symmetric about the centre of diffraction viz. y=0. The diffracted intensity exhibits<br />

2 2 2 2<br />

maxima equal to y 1 / ( t ) 1<br />

<br />

<br />

2 2<br />

m S m S<br />

m<br />

at angles y=y m satisfying the condition,<br />

S<br />

tan t y 1 / t y 1 / . The H and O intensities have been plotted in Fig.6 for<br />

t=20.25Δ S . Both the intensities oscillate strongly, the oscillations becoming more rapid in the<br />

29

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