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Examples and explanations of multiple integrals and vector calculus, focusing on changing the order of integration, change of variables, and vector products. It includes figures and formulas to illustrate the concepts.
Typology: Study notes
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Let’s review this subject by doing various examples of integrating a function f (x, y)
over a region of 2-space:
Ex. 1:
region
y
xdydx =
4
0
dx
x
√
x
0
y dy =
4
0
dx
x ·
x =
x
y
y=x
1/
2
4
Figure 1: Ex. 1
Q: how about changing the order of integration? We could do the x-integral
first obviously. But we need to be careful of the order of the limits.:
2
y=
dy y
4
x=y
2
x dx =
Q: Why change the order? Sometimes it’s important:
Ex. 2:
ln 16
x=
dx
4
y=e x/ 2
dy
ln y
Can’t do
dy/ ln y, so switch:
x
y
y=e
x/
4
Figure 2: Ex. 1
So let’s draw a new figure (always draw a figure if you switch!).
4
y=
dy
ln y
2 ln y
0
dx =
4
y=
dy · 2 = 6 (5)
First, let’s do a standard example where we don’t get into formalities:
x
y
dr
rd θ
1
1
dθ
y= (^) 1-x
2
Figure 3: Ex. 1
Ex. 3:
1
x=
√
1 −x 2
y=
e
−(x
2 +y
2 ) dydx (6)
Figure 4: Ex. 5. Original and transformed regions.
is to calculate Jacobian:
u, v
x, y
−y/x
2 1 /x
x + y
x
2
x, y
u, v
x
2
x + y
So
ve
v
x
2 (v)
x
2 (v)
v
dudv =
e
v dudv, (15)
nice and simple, but what are the transformed limits? Well, starting from the
original ones, we learn
y = 0 ⇒ u = 0 if x 6 = 0 ; y = x ⇒ u = 1 (16)
x = 1 ⇒ v = 1 + u ; y = x = 0 ⇒ v = 0. (17)
So
1
0
du
1+u
0
dv e
1
0
du(e
1+u − 1) = e
2 − e − 1. (18)
measures for cylindrical and spherical coords.: (Derived in Boas)–check!
Spherical x = r sin θ cos φ ; y = r sin θ sin φ ; z = r cos θ:
x, y, z
r, θ, φ
= r
2 sin θ (19)
i.e. dxdydz → r
2 sin θdrdθdφ (20)
Cylindrical x = ρ cos θ ; y = ρ sin θ; z = z :
x, y, z
ρ, θ, z
= ρ (21)
i.e. dxdydz → ρdρdθdz (22)
(N.B. θ in spherical coords. is not the same θ as for cylindrical coords!
Might want to use φ for cylindrical coords instead.)
Ex. 6:
Calculate the moment of inertia of a cone of height equal to its base radius
h = R. Take the density of the material to be ρ 0
, assumed homogeneous. Moment
of inertia is then
V
ρ 0 dV (x
2
2 ) = ρ 0
h
z=
dz
z
r=
rdr
2 π
0
dθ r
2 = ρ 0
πh
5
Note dimensions are correct, since [ρ 0
3 , so [ρ 0
h
5 ] = M L
2 .
4.3.1 Properties of vectors
Vector: “set of components which transforms under rotation of a coordinate system
in the same way as the coordinates of a point ~r. ” (“A vector is something that
transforms like a vector”.) Huh? What does that mean? Take the coordinates
x 1 , x 2 of a point ~r in a Cartesian coordinate system.
Figure 5: Transformation of coordinates x 1 , x 2 → x
′
1
, x
′
2
.
If we rotate the coordinate axes to a new set x
′
1
, x
′
2
by an angle φ, geometry tells
i
i
i
i
i
A = (aA 1
, aA 2
,... aA N
1
2 , · · · − aA N
B) = a
A + b
etc.
Magnitude of a vector:
N ∑
i=
2
i
N ∑
i=
′ 2
i
check! (39)
2 = A (40)
4.3.2 Products of vectors
i
i
i
i
jk
ijk
j
k
where ≤ ijk is the so-called Levi-Civita symbol, sometimes called the completely
antisymmetric tensor:
ijk
0 if any two indices are the same
+1 if indices correspond to an even permutation of 123
− 1 if indices correspond to an odd permutation of 123
Very useful identity – worth memorizing!
k
ijk
lmk = δ iδ jm − δ im δ j
Ex 1:
i
i
i
i
jk
ijk
j
k
`m
i`m
`
m
ijk`m
ijk
i`m
j
k
`
m
jk`m
(δ jδ km − δ jm δ k
j
k
`
m
`m
`
m
`
m
m
`
`
m
`
`
`
m
m
m
`
`
`
m
m
m
Some more identities to check using these techniques:
B) (“ BAC -CAB rule”)
Remarks:
B = AB cos θ AB
. If
B = 0, two vectors are “orthogonal”,
θ AB
= π/2.
note ˆe i × eˆ j
ijk ˆe k
A in terms of D orthogonal unit vectors in D dimensions,
i
i eˆ i
formations:
′ ·
i
′
i
′
i
i
j
a ij
i
k
a ik
k
ijk
a ij a ik
j
k
jk
δ jk
j
k
k
k
k
B| = AB sin θ AB