The first figure shows the 4 possible cases for reflection and transmission at
an interface. Lets solve the problem, which is shown in the next figure
since
μ
1
≠
μ
2
μ
1
≠
μ
2
it must be that
v
1
≠
1
≠
v
2
2
.
Note that we are assuming that Young's Modulus is constant across the
boundary.
So we get
y
i
n
c
=
A
cos
(
k
1
x
−
ω
t
)
y
i
n
c
=
A
cos
(
k
1
x
−
ω
t
)
y
r
e
f
=
B
cos
(
k
1
x
+
ω
t
)
y
r
e
f
=
B
cos
(
k
1
x
+
ω
t
)
y
t
r
a
n
s
=
C
cos
(
k
2
x
−
ω
t
)
y
t
r
a
n
s
=
C
cos
(
k
2
x
−
ω
t
)
(note
the reflected wave goes the other direction).
On the left side of the junction we
have
y
l
=
y
i
n
c
+
y
r
e
f
=
A
cos
(
k
1
x
−
ω
t
)
+
B
cos
(
k
1
x
+
ω
t
)
y
l
=
y
i
n
c
+
y
r
e
f
=
A
cos
(
k
1
x
−
ω
t
)
+
B
cos
(
k
1
x
+
ω
t
)
and on the right side of the junction we have
y
r
=
y
t
r
a
n
s
=
C
cos
(
k
2
x
−
ω
t
)
.
y
r
=
y
t
r
a
n
s
=
C
cos
(
k
2
x
−
ω
t
)
.
At the boundary
x
=
0
x
=
0
the wave must continuous, that is there are no kinks in it. Thus we must have
y
l
(
0
,
t
)
=
y
r
(
0
,
t
)
y
l
(
0
,
t
)
=
y
r
(
0
,
t
)
∂
y
l
(
x
,
t
)
∂
x
|
x
=
0
=
∂
y
r
(
x
,
t
)
∂
x
|
x
=
0
∂
y
l
(
x
,
t
)
∂
x
|
x
=
0
=
∂
y
r
(
x
,
t
)
∂
x
|
x
=
0
So from the first equation
A
cos
(
ω
t
)
+
B
cos
(
ω
t
)
=
C
cos
(
ω
t
)
A
cos
(
ω
t
)
+
B
cos
(
ω
t
)
=
C
cos
(
ω
t
)
A
+
B
=
C
A
+
B
=
C
∂
y
l
(
x
,
t
)
∂
x
|
x
=
0
=
∂
y
r
(
x
,
t
)
∂
x
|
x
=
0
∂
y
l
(
x
,
t
)
∂
x
|
x
=
0
=
∂
y
r
(
x
,
t
)
∂
x
|
x
=
0
−
A
k
1
sin
(
−
ω
t
)
−
k
1
B
sin
(
ω
t
)
=
−
k
2
C
sin
(
−
ω
t
)
−
A
k
1
sin
(
−
ω
t
)
−
k
1
B
sin
(
ω
t
)
=
−
k
2
C
sin
(
−
ω
t
)
(
A
−
B
)
k
1
sin
ω
t
=
C
k
2
sin
ω
t
(
A
−
B
)
k
1
sin
ω
t
=
C
k
2
sin
ω
t
A
−
B
=
k
2
k
1
C
A
−
B
=
k
2
k
1
C
now
solve for
B
B
and
C
C
A
+
B
=
C
A
+
B
=
C
A
−
B
=
k
2
k
1
C
A
−
B
=
k
2
k
1
C
2
A
=
(
1
+
k
2
k
1
)
C
2
A
=
(
1
+
k
2
k
1
)
C
Thus
we can define the transmission coefficient
t
r
≡
C
/
A
=
2
k
1
k
1
+
k
2
t
r
≡
C
/
A
=
2
k
1
k
1
+
k
2
and
the refection coefficient
r
≡
B
/
A
=
C
A
−
1
=
k
1
−
k
2
k
1
+
k
2
r
≡
B
/
A
=
C
A
−
1
=
k
1
−
k
2
k
1
+
k
2
note
how the amplitudes can change at the boundary
If
μ
2
<
μ
1
μ
2
<
μ
1
then
we must have
k
2
<
k
1
k
2
<
k
1
since
v
=
ω
/
k
=
T
/
μ
v
=
ω
/
k
=
T
/
μ
and
ω
ω
and
T
T
must be fixed. We see that
k
∝
μ
k
∝
μ
In this case we see that the amplitude of the wave gets bigger when it moves
into a less dense medium. We have probably all experienced this in real
life. As waves come ashore they become bigger. This is because shallower
water is effectively less dense. A tsumami in open ocean may have an
imperceptable amplitude but when it comes ashore it can be tremendous. This
seems almost counter intuitive, but in any closed system the energy and power
are conserved but there is no rule saying amplitude has to be conserved.
Lets look at the reflected and transmitted power. Recall Power:
P
=
1
2
μ
ω
2
A
2
v
P
=
1
2
μ
ω
2
A
2
v
For the incident and reflected waves
μ
μ
and
ν
ν
are the same so the reflected power coefficient (reflected power / incident
power)
P
R
=
(
B
/
A
)
2
=
(
k
1
−
k
2
k
1
+
k
2
)
2
P
R
=
(
B
/
A
)
2
=
(
k
1
−
k
2
k
1
+
k
2
)
2
To do transmitted power lets first rewrite the power equation. Recall
v
=
ν
λ
=
2
π
ν
k
=
ω
k
v
=
ν
λ
=
2
π
ν
k
=
ω
k
Also
v
=
T
μ
v
=
T
μ
so
μ
=
T
v
2
=
T
(
ω
k
)
2
=
T
k
2
ω
2
μ
=
T
v
2
=
T
(
ω
k
)
2
=
T
k
2
ω
2
so now
P
=
1
2
μ
ω
2
A
2
v
P
=
1
2
μ
ω
2
A
2
v
becomes
P
=
1
2
T
k
2
ω
2
ω
2
A
2
ω
k
P
=
1
2
T
k
2
ω
2
ω
2
A
2
ω
k
or
P
=
1
2
T
k
ω
A
2
.
P
=
1
2
T
k
ω
A
2
.
Watch out, in the above lines A was used to denote amplitude in general
and in the following line it specifically refers to the incoming wave.
The
transmission power coefficient is thus:
P
T
=
1
2
T
k
2
ω
C
2
1
2
T
k
1
ω
A
2
P
T
=
1
2
T
k
2
ω
C
2
1
2
T
k
1
ω
A
2
Note that
ω
ω
and
T
T
are the same for both waves
P
T
=
k
2
C
2
k
1
A
2
P
T
=
k
2
C
2
k
1
A
2
earlier we showed
C
/
A
=
2
k
1
k
1
+
k
2
C
/
A
=
2
k
1
k
1
+
k
2
so
P
T
=
(
2
k
1
k
1
+
k
2
)
2
k
2
k
1
P
T
=
(
2
k
1
k
1
+
k
2
)
2
k
2
k
1
P
T
=
4
k
1
k
2
(
k
1
+
k
2
)
2
P
T
=
4
k
1
k
2
(
k
1
+
k
2
)
2
Note that
P
R
+
P
T
=
1
P
R
+
P
T
=
1
which means that energy is conserved.
Now lets look at the 4 specific cases we have:
Rigid wall
μ
→
∞
μ
→
∞
so
k
2
→
∞
k
2
→
∞
r
=
k
1
−
k
2
k
1
+
k
2
=
k
1
k
2
−
1
k
1
k
2
+
1
r
→
−
1
r
=
k
1
−
k
2
k
1
+
k
2
=
k
1
k
2
−
1
k
1
k
2
+
1
r
→
−
1
Also
P
R
→
+
1
P
R
→
+
1
P
T
→
0
P
T
→
0
So wave is reflected and inverted, but has same power
Free end
μ
→
0
μ
→
0
so
k
2
→
0
k
2
→
0
r
=
k
1
−
k
2
k
1
+
k
2
=
k
1
k
1
r
→
+
1
r
=
k
1
−
k
2
k
1
+
k
2
=
k
1
k
1
r
→
+
1
Also
P
R
→
+
1
P
R
→
+
1
P
T
→
0
P
T
→
0
So wave is reflected and has same power
Moving to higher density
μ
2
>
μ
1
k
2
>
k
1
μ
2
>
μ
1
k
2
>
k
1
so
r
<
0
r
<
0
t
r
>
0
t
r
>
0
Moving to lower density
μ
2
<
μ
1
k
2
<
k
1
μ
2
<
μ
1
k
2
<
k
1
so
r
>
0
r
>
0
t
r
>
1
t
r
>
1
Note the transmitted wave's amplitude is larger than the original.
"This book covers second year Physics at Rice University."