Digital Signal Processing Reference
In-Depth Information
25
20
15
10
5
0
0.5
0.5
0
0
-0.5
-0.5
Figure 2.13 . The pdf of Eq. (2.21) plotted for σ e =0 . 01.
The probability of error in detection of the QAM symbol is therefore
−P e,P AM ( b/ 2)) 2 ,
P e,QAM ( b )=1
(1
(2 . 24)
where we have used the functional arguments to indicate the number of bits.
Thus
P e,P AM ( b/ 2) is the error probability for a ( b/ 2)-bit PAM constellation
with energy E ave and noise variance σ e . For small errors the preceding equation
can be approximated as
1
P e,P AM ( b/ 2)
P e,QAM ( b )=1
2
P e,P AM ( b/ 2) +
2
P e,P AM ( b/ 2) , (2 . 25)
where we have neglected
P e,P AM ( b/ 2). This approximation is quite reasonable
in practice. For example, even if
P e,P AM ( b/ 2) = 10 3 (a rather large value), its
square is 10 6 , which can be neglected. Thus the error probability for the QAM
constellation can be approximated by
3 E ave
(2 b
,
2 −b/ 2 )
P e,QAM ( b )
2
P e,P AM ( b/ 2)=4(1
Q
(2 . 26)
1) σ e
where b isthenumberofbits, E ave is the average energy of the constellation,
and σ e is the variance of the complex Gaussian error term e ( n ) at the input of
the detector. For comparsion, recall that a b -bit PAM constellation with the
same energy E ave and noise variance σ e
would have error probability
3 E ave
(2 2 b
.
2 −b )
P e,P AM ( b ) = 2(1
Q
(2 . 27)
1) σ e
 
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