
23 8 
Chapter 2 
where  Eq.  2.129  is  forward  (-i)  and  Eq.  2.128  is  reverse  (+i)  Fourier 
transforms. Here, @(h) is the function defined in the reciprocal space, i.e. the 
scattered amplitude; p(x) is the corresponding function defined in the direct 
space,  e.g.  p(x)  is  the  electron  density when  scattering of  x-rays  is  of 
concern or it is the nuclear density when scattering of neutrons on nuclei is 
considered; h and x are the coordinate vectors in the reciprocal and direct 
spaces, respectively; 
V* 
and 
V 
are, respectively, reciprocal and direct space 
volumes, and 
i 
= 
fi 
. 
Both integrals do not require assumption of periodicity and they can be 
used  to  calculate  the  scattered  amplitude  or  the  corresponding  density 
function of any direct or reciprocal object, respectively. For example, Eq. 
2.128 results  in the atomic scattering factor, 
flsinelh) 
cc 
I@(h)l, when the 
integration  is  performed  for  an  isolated  atom. 
In 
this  case,  p(x)  is  the 
electron density distribution in  the  atom, which is  usually  obtained from 
quantum mechanics. 
Considering a crystal, in which the electron density function is periodic, 
the integral in Eq. 2.128 can be substituted by a sum: 
F(h) 
= 
v 
p(x) 
exp[2ni(h 
. 
x)] 
X 
where P(h) is the structure amplitude at a reciprocal lattice point h, 
V 
is the 
volume of the unit cell of the direct lattice and the summation is carried over 
all possible coordinate vectors, x, in the unit cell for a specific h. 
When Eq. 2.130 is compared with Eq. 2.87,  it is easy to  see that the 
distribution of the electron density in the unit cell is modeled by 
n products, 
g'P(sinelhlfJ(sinelh), where 
g', 
P 
and 
f 
j 
are the population, temperature and 
scattering factors of  the 
jth 
atom, respectively, and the  summation ranges 
over all atoms (from 1 to n) that are present in the unit cell. 
Similar substitution of the forward Fourier integral (Eq. 2.129) results in 
the following sum, which enables one to calculate the distribution of the 
electron  (or  nuclear)  density  in  the  unit  cell  from  the  known  structure 
amplitudes: 
1 
p(x) 
= 
- 
~(h) exp[-  2ni(h 
. 
x)] 
v 
h 
Here the summation is carried over all reciprocal lattice points, h, for a 
given  coordinate  vector, 
x. 
The  last  equation  has  exceptional practical 
importance as it allows one to convert the array of numbers 
- 
the observed 
structure amplitudes obtained from the experimentally measured intensities 
-