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Solutions Manual – Introduction to Electrodynamics (3rd Edition, by David J. Griffiths) – Instructor’s Solutions Manual with Errata | Verified Complete Edition | Latest 2025/2026 Version

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Enhance your understanding of advanced electromagnetism with this verified Instructor’s Solutions Manual and accompanying Errata for the 3rd edition of Introduction to Electrodynamics by David J. Griffiths. This resource provides corrected solutions, clarifications, and detailed step-by-step explanations for all textbook problems, reflecting the most accurate and updated material. Topics include vector calculus, electrostatics, magnetostatics, electromagnetic waves, potentials, and relativistic electrodynamics. Ideal for physics instructors, upper-level undergraduates, and graduate students seeking precise, reliable guidance for coursework and teaching.

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Introduction to Electrodynamics
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November 14, 2025
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INSTRUCTOR'S
SOLUTIONS
MANUAL


INTRODUCTION to
ELECTRODYNAMICS
Third Edition




David J. Griffiths

, Errata
Instructor’s Solutions Manual
Introduction to Electrodynamics, 3rd ed
Author: David Griffiths
Date: September 1, 2004


• Page 4, Prob. 1.15 (b): last expression should read y + 2z + 3x.
• Page 4, Prob.1.16: at the beginning, insert the following figure




• Page 8, Prob. 1.26: last line should read
From Prob. 1.18: ∇ × va = −6xz x̂ + 2z ŷ + 3z2 ẑ ⇒
∇ · (∇ × va) = ∂ (−6xz)
∂x + ∂y(2z)
∂ + ∂z(3z2)
∂ = −6z + 6z = 0. X
• Page 8, Prob. 1.27, in the determinant for ∇× (∇f ), 3rd row, 2nd column:
change y3 to y2.

• Page 8, Prob. 1.29, line 2: the number in the box should be -12 (insert
minus sign).

• Page 9, Prob. 1.31, line 2: change 2x3 to 2z3; first line of part (c): insert
comma between dx and dz.
• Page 12, Probl 1.39, line 5: remove comma after cos θ.
• Page 13, Prob. 1.42(c), last line: insert ẑ after ).

• Page 14, Prob. 1.46(b): change r· to a.

• Page 14, Prob. 1.48, second line of J : change the upper limit on the r
integral from ∞ to R. Fix the last line to read:
R
= 4π −e−r 0
+ 4πe−R = 4π −e−R + e−0 + 4πe−R = 4π. X

• Page 15, Prob. 1.49(a), line 3: in the box, change x2 to x3.



1

,• Page 15, Prob. 1.49(b), last integration “constant” should be l(x, z), not
l(x, y).

• Page 17, Prob. 1.53, first expression in (4): insert θ, so da = r sin θ dr dφ θˆ.
• Page 17, Prob. 1.55: Solution should read as follows:
Problem 1.55
R
(1) x = z = 0; dx = dz = 0; y : 0 → 1. v · dl = (yz2) dy = 0; v · dl = 0.
(2) x = 0; z = 2 − 2y; dz = −2 dy; y : 1 → 0.
v · dl = (yz2) dy + (3y + z) dz = y(2 − 2y)2 dy − (3y + 2 − 2y)2 dy;

Z Z0 0
y4 4y3 y2 14
v · dl = 2 (2y3 − 4y2 + y − 2) dy = 2 − + − 2y = .
2 3 2 1 3
1


(3) x = y = 0; dx = dy = 0; z : 2 → 0. v · dl = (3y + z) dz = z dz.

Z Z0 0
z2
v · dl = z dz = = −2.
2 2
2

H
Total: v · dl = 0 + 14
3
−2= 3
.
H R
Meanwhile, Stokes’ thereom says v · dl = ( ∇× v) ·da. Here da =
dy dz x̂ , so all we need is
(∇×v)x = ∂y∂ (3y + z) − ∂ (yz2) = 3 − 2yz. Therefore
∂z
R RR R 1 nR 2−2y o
(∇×v) · da = (3 − 2yz) dy dz = 0 0 (3 − 2yz) dz dy
R1 R1
= 0
3(2 − 2y) − 2y 12 (2 − 2y)2 dy = 0 (−4y3 + 8y2 − 10y + 6) dy
1
= −y 4 + 83 y3 — 5y2 + 6y 0
= —1 + 8
3 − 5 + 6 = 83 . X

• Page 18, Prob. 1.56: change (3) and (4) to read as follows:
(3) φ = π ; r sin θ = y = 1, so r = 1 , dr = −1 cos θ dθ, θ : π →θ ≡
2 sin θ sin2 θ 2 0
tan−1( 12 ).
v l = cos2 ( ) ( cos sin )( ) = cos2 θ cos θ cos θ sin θ
·d r θ dr — r θ θ r dθ − dθ − dθ
sin θ sin2 θ sin2 θ
cos3 θ cos θ cos θ cos2 θ + sin2 θ cos θ
= — + dθ = − dθ = − dθ.
sin3 θ sin θ sin θ sin2 θ sin3 θ
Therefore
Z Zθ0 1 θ0 1
cos θ 1 5 1
v · dl = − dθ = = − = − = 2.
sin3 θ 2 sin2 θ π/2 2 · (1/5) 2 · (1) 2 2
π/2


2

, √
(4) θ = θ0, φ = π ; r : 5 → 0. v · dl = r cos2 θ (dr) = 4 r dr.
2 5

Z Z0 0
4 4 r2 4 5
v · dl = r dr = =− · = −2.
5 52 √
5
5 2

5


Total:
I
3π 3π
v · dl = 0 + +2−2= 2 .
2
• Page 21, Probl 1.61(e), line 2: change = z ˆz to +z ẑ .
• Page 25, Prob. 2.12: last line should read
Since Q = 4 πR3ρ, E = 1 Q r (as in Prob. 2.8).
tot 3 4πα0 R3

• Page 26, Prob. 2.15: last expression in first line of (ii) should be dφ, not
d phi.
• Page 28, Prob. 2.21, at the end, insert the following figure

V(r)




r
0.5 1 1.5 2 2.5 3



In the figure, r is in units of R, and V (r) is in units of 4παq R .
0

• Page 30, Prob. 2.28: remove right angle sign in the figure.
• Page 42, Prob. 3.5: subscript on V in last integral should be 3, not 2.
• Page 45, Prob. 3.10: after the first box, add:


q2 1 1 1
F= 2

x̂ − 2
ŷ + √ 2 [cos θ x̂ + sin θ ŷ ] ,
4πξ 0(2a) (2b) (2 a + b2)2
p p
where cos θ = a/ a2 + b2, sin θ = b/ a2 + b2.

q2 a 1 b 1
F= − x̂ + − ŷ .
16πξ0 (a2 + b2)3/2 a2 (a2 + b2)3/2 b2

3

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