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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