Prof. David R. Jackson ECE Dept. Spring 2014 Notes 30 ECE 6341 1.
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Prof. David R. Jackson Dept. of ECE
Spring 2018
Notes 10 Gauss’s Law I
ECE 3318 Applied Electricity and Magnetism
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Notes prepared by the EM Group University of Houston
Gauss’s Law
Assume q produces Nf flux lines
qψ =
A charge q is inside a closed surface.
Hence
NS = Nf (all flux lines go through S)
Sf
q NN
ψ
=
2
NS ≡ # flux lines that go through S
ˆS
D n dSψ ≡ ⋅∫
From the picture:
S (closed surface)
ˆ ( )n outward normal
x
y
z
E
q
Gauss’s Law (cont.)
NS = 0
ˆ 0S
D n dSψ = ⋅ =∫
The charge q is now outside the surface
(All flux lines enter and then leave the surface.)
Hence
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qS
To summarize both cases, we have Gauss’s law:
ˆ enclS
D n dS Q⋅ =∫
By superposition, this law must be true for arbitrary charges.
Gauss’s Law (cont.)
Carl Friedrich Gauss
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n̂ = outward normal
(his signature)
Example
1 2 3
ˆ ˆ ˆ0 2S S S
D n dS q D n dS D n dS q⋅ = ⋅ = ⋅ =∫ ∫ ∫
Note: All of the charges contribute to the electric field in space.
Note: E ≠ 0 on S2 !
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1S2S
3S
2qq−q
Using Gauss’s Law
Gauss’s law can be used to obtain the electric field
for certain problems.
The problems must be highly symmetrical.
⇒ The problem must reduce to one unknown field component (in one of the three coordinate systems).
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Note: When Gauss’s law works, it is usually easier to use than Coulomb’s law
(i.e., the superposition formula).
Choice of Gaussian Surface
Rule 1: S must be a closed surface.
Guideline: Pick S to be ⊥ to E as much as possible
ˆ (LHS)S
D n dS= ⋅∫Left -hand side
ˆS E n D⊥ ⇒
Rule 2: S should go through the observation point (usually called r).
(This simplifies the dot product calculation.)
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ˆ enclS
D n dS Q⋅ =∫
n̂
E
S
Example
Find E
Point charge
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q
x
y
z
Example (cont.)
Assume
ˆ enclS
D n dS Q q⋅ = =∫
Assume
( )r rD D r=
ˆ rD r D=
( )ˆ ˆrS
rS
D r r dS q
D dS q
⋅ =
=
∫
∫
rS
D dS q=∫9
(only a function of r)
(only an r component)
( )24rD r qπ =or Then
ˆ ˆn r=
S
q
r
x
y
z
r
Example (cont.) We then have
( )2
2
4
4
r
r
D r q
qDr
π
π
=
=
20
ˆ4
qE rrπε
=
Hence
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so
22 C/mˆ
4qD rrπ
=
( )2ˆLHS 4rS
D n dS D rπ= ⋅ =∫
RHS enclQ q= =
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q
x
y
z
[ ]20
V/mˆ4
qE rrπε
=
Example (cont.)
Summary
Note About Spherical Coordinates Note: In spherical coordinates, the LHS is always:
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( )2ˆ ˆLHS 4r rS S S
D n dS D r dS D dS D rπ= ⋅ = ⋅ = =∫ ∫ ∫
( )ˆ ˆ( )r rD r D r r θ φ= in the direction, and a function of only, not and
( ) ( ), , ( )v rr f r θ φρ θ φ = a function of only, not and
Assumption:
( )2LHS 4rD rπ=
Example
Find E everywhere
Hollow shell of uniform surface charge density
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x
y
z
0s sρ ρ=
a
Example (cont.)
( )24 0r enclD r Qπ = =
V/m0 [ ]E =
Case a) r < a
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Hence
0rD =so
LHS = RHS
x
y
z
0s sρ ρ=
a
a
0sρ
rr
Example (cont.)
( )2 20
20
2
2
4 4
44
4
r encl s
sr
r
D r Q a
aDr
QDr
π ρ π
π ρπ
π
= =
⇒ =
⇒ =
Case b) r > a
20
V/mˆ [ ]4
QE rrπε
=
The electric field outside the sphere of surface charge is the same as from a point charge at the origin.
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Hence
LHS = RHS
ar
0sρ
r
Example (cont.)
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V/mˆ [ ]4
QE rrπε
=
V/m0 [ ]E =
Note: A similar result holds for the force due to gravity from a
shell of material mass.
Summary
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x
y
z
0s sρ ρ=
a r a>
r a<
Example (cont.)
Note: The electric field is discontinuous as we cross the boundary of a surface
charge density.
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204
Qrπε
x
y
z
0s sρ ρ=
a
ar
rE
( )20/ 4Q aπε
Example
Find E(r) everywhere
Solid sphere of uniform volume charge density
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x
y
z
0v vρ ρ=
a
Example (cont.)
( )2
ˆ
4
enclS
r encl
D n dS Q
D r Qπ
⋅ =
⇒ =
∫
Case a) r < a
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( )encl vV
Q r dVρ= ∫
x
y
z
0v vρ ρ=
a
Gaussian surface S
rr
a0vρ
Example (cont.)
0
0
30
43
encl vV
vV
v
Q dV
dV
r
ρ
ρ
ρ π
=
=
=
∫
∫
Calculate RHS:
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( )2 30
443r vD r rπ ρ π =
LHS = RHS
Gaussian surface S
rr
a0vρ
Example (cont.)
00
V/mˆ [ ]3vrE r ρε
=
013r vD rρ =
Hence, we have
The vector electric field is then:
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x
y
z
0v vρ ρ=
a
r a<
r
Example (cont.)
so
30
43encl vQ aρ π =
Case b) r > a
[ ]3
02
0
V/mˆ3
v aE rr
ρε
=
Hence, we have
22
( )2
ˆ
4
enclS
r encl
D n dS Q
D r Qπ
⋅ =
⇒ =
∫
( )2 30
3
0 2
443
3
r v
r v
D r a
aDr
π ρ π
ρ
=
⇒ =
Gaussian surface S
a r
r
0v vρ ρ=
Example (cont.) We can write this as:
The electric field outside the sphere of charge is the same as from a
point charge at the origin.
30
43vQ aρ π =
( )( )
30
20
4 / 3ˆ
3 4 / 3v aE r
rπρ
ε π
=
20
ˆ4
QE rrπε
=
where
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Hence
x
y
z
0v vρ ρ=
a
r a>
r
Example (cont.)
00
V/mˆ [ ]3vrE r ρε
=
[ ]3
02 2
0 0
V/mˆ ˆ3 4
v a QE r rr r
ρε πε
= =
Summary
Note: The electric field is continuous as we
cross the boundary of a volume charge density.
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x
y
z
0v vρ ρ=
a
ra
rE
( )0 0/ 3v aρ ε
r a>
r a<