Another important channel model occurs when the
signal is uncorrupted save for the addition of Gaussian noise that
is not necessarily white or stationary. We presume that
correlation function of the noise is known. In particular we
model the production of
nt
n
t
by passing white, Gaussian noise
ωt
ω
t
through a linear filter.
(Figure 1)
We can convert this detection problem to one we
have solved. Namely assume the existence of a whitening filter
h
ω
tτ
h
ω
t
τ
that changes
nt
n
t
into a white process. Consider passing
rt
r
t
through this whitening filter.
(Figure 2)
This procedure does not remove signal information as the
whitening filter is reversible. We assume that
R
ω
tu=δt-u
R
ω
t
u
δ
t
u
. We then have the detection of a known signal in white,
Gaussian noise. We have solved this problem
previously and know the minimum
P
e
P
e
receiver computes the quantity
ln
π
i
+<
Q
n
,r>-∥si∥
Q
n
22
π
i
Q
n
r
s
i
Q
n
s
i
2
2
where
<
Q
n
,r>=∫∫rt
s
i
u
Q
n
tudtdu
Q
n
r
s
i
u
t
r
t
s
i
u
Q
n
t
u
and
Q
n
tu=∫
h
ω
αt
h
ω
αudα
Q
n
t
u
α
h
ω
α
t
h
ω
α
u
. Consequently, all of the issues and solutions
involved with the dispersive channel problem arise here. For
example, antipodal signals are optimum. However, we shall see
that there is a possibility of having communication over a noisy
channel with no error!
The inner product term
<
Q
n
,r>
Q
n
r
s
i
can be written as a matched filter.
∫∫rt
s
i
u
Q
n
tudtdu=∫rt
g
i
tdt
u
t
r
t
s
i
u
Q
n
t
u
t
r
t
g
i
t
where we define
g
i
t
g
i
t
as
∫
s
i
u
Q
n
tudu
u
s
i
u
Q
n
t
u
. To find
g
i
t
g
i
t
more directly, we note that the correlation function
of the output of the whitening filter is given by
∫∫
h
ω
tα
h
ω
uβ
K
n
αβdαdβ=δt-u
β
α
h
ω
t
α
h
ω
u
β
K
n
α
β
δ
t
u
Convolving both sides of this equation with
h
ω
tv
h
ω
t
v
, we have
∫
h
ω
tvdt∫∫
h
ω
tα
h
ω
uβ
K
n
αβdαdβ=
h
ω
uv
t
h
ω
t
v
β
α
h
ω
t
α
h
ω
u
β
K
n
α
β
h
ω
u
v
Interchanging the order of integration results in
∫
h
ω
uβ∫
Q
n
αv
K
n
αβdαdβ=
h
ω
uv⇒∫
Q
n
αv
K
n
αβdα=δv-β
β
h
ω
u
β
α
Q
n
α
v
K
n
α
β
h
ω
u
v
α
Q
n
α
v
K
n
α
β
δ
v
β
Because of this property, we can have that for any choice of
φ
i
t
φ
i
t
∫
φ
i
β∫
Q
n
αv
K
n
αβdαdβ=
φ
i
v
β
φ
i
β
α
Q
n
α
v
K
n
α
β
φ
i
v
Let
φ
i
t
φ
i
t
denote the eigenfunctions of
K
n
αβ
K
n
α
β
. In this case, by interchanging integration order, we
find that
∫
Q
n
αv
φ
i
αdα=1
λ
i
φ
i
v
α
Q
n
α
v
φ
i
α
1
λ
i
φ
i
v
Consequently, eigenfunctions of
K
n
K
n
are also eigenfunctions of
Q
n
Q
n
, and the eigenvalues are reciprocals of each other.
Q
n
Q
n
is thus termed the inverse kernel of
K
n
K
n
. Using Mercer's Theorem,
K
n
tu=∑
λ
i
φ
i
t
φ
i
u
K
n
t
u
λ
i
φ
i
t
φ
i
u
Q
n
tu=∑1
λ
i
φ
i
t
φ
i
u
Q
n
t
u
1
λ
i
φ
i
t
φ
i
u
Recalling the defining
equation for
g
i
t
g
i
t
, multiplying by
K
n
tβ
K
n
t
β
and integrating
∫
K
n
tβ
g
i
βdβ=∫∫
s
i
u
Q
n
βu
K
n
tβdudβ=∫
s
i
udu∫
Q
n
βu
K
n
tβdβ
β
K
n
t
β
g
i
β
β
u
s
i
u
Q
n
β
u
K
n
t
β
u
s
i
u
β
Q
n
β
u
K
n
t
β
(1)
As
Q
n
··
Q
n
·
·
is the inverse kernel of
K
n
··
K
n
·
·
the last integral equals an impulse, and the impulse
response
g
i
t
g
i
t
of the optimum receiver's matched filter is the
solution of the integral equation
∫
K
n
tβ
g
i
βdβ=
s
i
t
β
K
n
t
β
g
i
β
s
i
t
Despite the fact that this is an implicit equation for
g
i
t
g
i
t
, it is easier to solve than the explicit equation
given above. The reason is that one is usually given the noise
covariance function rather than its inverse kernel.
Generally, one assumes the covariance function of
the noise to be
K
n
tu=
N
0
2δt-u+
K
c
tu
K
n
t
u
N
0
2
δ
t
u
K
c
t
u
where
K
c
tu
K
c
t
u
denotes the colored noise component of
K
n
tu
K
n
t
u
[
K
c
tu
K
c
t
u
has no impulses]. The equation for
g
i
t
g
i
t
becomes
N
0
2
g
i
t+∫
K
c
tu
g
i
udu=
s
i
t
N
0
2
g
i
t
u
K
c
t
u
g
i
u
s
i
t
(2)
This expression is the Fredholm integral equation of
the second kind. If
N
0
=0
N
0
0
(no white noise), we have the Fredholm integral of the
first kind. Assume that
nt
n
t
is stationary; this situation implies that its
covariance function has the form
K
n
tu=
K
n
t-u=
N
0
2δt-u+
K
c
t-u
K
n
t
u
K
n
t
u
N
0
2
δ
t
u
K
c
t
u
As we shall see, the absence or presence of the white
noise term (
i.e., does
𝒮
n
f→0
𝒮
n
f
0
as
f→∞
f
or not) has a pronounced effect on the nature of
g
i
t
g
i
t
. In general, if
N
0
=0
N
0
0
, the solution will contain impulses, and, furthermore,
the performance of the receiver will be
very sensitive to assumptions one makes
about the noise. If
N
0
≠0
N
0
0
, the character of
g
i
t
g
i
t
changes completely: Answers make more sense, and the
results are "nicer."
To make these considerations more precise, we consider the
important special case where
𝒮
n
f
𝒮
n
f
is a rational function.
𝒮
n
f=N2πf2D2πf2
𝒮
n
f
N
2
f
2
D
2
f
2
where
N·
N
·
and
D·
D
·
are polynomials. Because
ⅈ2πf
2
f
is associated with the derivative in the time domain,
we see that
K
n
τ
K
n
τ
satisfies the differential equation:
D-p2
K
n
τ=N-p2δτ
D
p
2
K
n
τ
N
p
2
δ
τ
where
p↔ddτ
↔
p
τ
,
p2↔d2dτ2
↔
p
2
τ
2
,
p3↔d3dτ3
↔
p
3
τ
3
, etc. Now, we wish to solve
s
i
t=∫0T
K
n
t-u
g
i
udu
s
i
t
u
0
T
K
n
t
u
g
i
u
Multiplying by
D-p2
D
p
2
, with pp representing
taking a derivative with respect to
tt,
D-p2
s
i
t=∫0TD-p2
K
n
t-u
g
i
udu
D
p
2
s
i
t
u
0
T
D
p
2
K
n
t
u
g
i
u
Using the differential equation given previously that the noise covariance
function must satisfy, we find that,
∀t,0≤t≤T:D-p2
s
i
t=∫0TN-p2δt-u
g
i
udu=N-p2
g
i
t
t
0
t
T
D
p
2
s
i
t
u
0
T
N
p
2
δ
t
u
g
i
u
N
p
2
g
i
t
(3)
Consequently, the solution to our integral equation
can be found by solving this differential equation. The solution
consists of the particular solution
g
i
P
t
g
i
P
t
and the homogeneous solution of
N-p2
g
i
t=0
N
p
2
g
i
t
0
.
When the observation interval is
finite, the solution may also contain impulses at the
boundaries.
Letting
nn denote
the order of the numerator polynomial and
mm the order of the denominator, the
solution has the form
gt=
g
P
t+∑i=12n
a
i
g
i
h
t+∑k=0m-n-1
b
k
δ
k
t-
T
i
+
c
k
δ
k
t-
T
f
g
t
g
P
t
i
1
2
n
a
i
g
i
h
t
k
0
m
n
1
b
k
δ
k
t
T
i
c
k
δ
k
t
T
f
If the impulses are not included, the original
integral equation may not be satisfied; this situation occurs
when
N
0
=0
N
0
0
. When
N
0
≠0
N
0
0
, the impulses are no longer necessary.
Additional "funny things" happen when
N
0
=0
N
0
0
. If, for example, an antipodal signal set is used,
∥s0-s1∥Q2=4∥s0∥Q2=∑j=1∞
s
0
j
2
λ
j
c
+
N
0
2
Q
s
0
s
1
2
4
Q
s
0
2
j
1
s
0
j
2
λ
j
c
N
0
2
where
λ
j
c
λ
j
c
is an eigenvalue of
K
c
tu
K
c
t
u
. When
N
0
≠0
N
0
0
,
s
0
j
2
λ
j
c
+
N
0
2≤
s
0
j
2
N
0
2
s
0
j
2
λ
j
c
N
0
2
s
0
j
2
N
0
2
, which means that this distance will always be
finite. On the other hand, if
N
0
=0
N
0
0
,
∑
s
0
j
2
λ
j
c
s
0
j
2
λ
j
c
may not converge. In such cases, the signals are
infinitely far apart with respect to the distance measure
induced by the inverse kernel, and the probability of error is
zero! Generally speaking, such behavior is not obtained in
actuality. White noise is usually present in the front end of a
receiver.
The colored noise component has power
density spectrum and covariance function given by
𝒮
c
f=2αββ2+2πf2
𝒮
c
f
2
α
β
β
2
2
f
2
K
c
τ=αⅇ-β|τ|
K
c
τ
α
β
τ
The differential equation to solve when
N
0
=0
N
0
0
becomes
-d2dt2
s
i
t+β2
s
i
t=2αβgt
t
2
s
i
t
β
2
s
i
t
2
α
β
g
t
Obviously, we have an explicit equation for
gt
g
t
, meaning that
g
h
t=0
g
h
t
0
. Adding in the impulses and substituting back into
the integral equation, the total solution is
gt=12αββs′0-s′0δt+βsT-s′Tδt-T+β2st-st′′
g
t
1
2
α
β
β
s
0
s
0
δ
t
β
s
T
s
T
δ
t
T
β
2
s
t
2
s
t
Note that if
st
s
t
is discontinuous, we have doublets in the signal
gt
g
t
! If, however,
N
0
≠0
N
0
0
, the differential equation becomes
N
0
2-d2dt2g+γ2gt=-d2dt2s+β2st
N
0
2
t
2
g
γ
2
g
t
t
2
s
β
2
s
t
where
γ2=β2+4αβ
N
0
γ
2
β
2
4
α
β
N
0
. Therefore,
g
h
t=
a
1
ⅇ-γt+
a
2
ⅇγt
g
h
t
a
1
γ
t
a
2
γ
t
and there are no impulses! Consequently, one usually
assumes the presence of some white noise to refrain from
obtaining rather bizarre answers.