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Formulas in Electrodynamics
Based on course by Yuri Lyubarsky and Edited By Eitan Rothstein
Department of Physics, Ben-Gurion University, Beer-Sheva 84105, Israel
1 p·r̂
Electric dipole moment potential Vdip (r) = 4π
2 , with the electric dipole moment p =
0 r
1 1
The electric field of an electric dipole is Edip (r) = 4π
3 [3(p · r̂) · r̂ − p].
0 r
µ0 1
The magnetic field of a magnetic dipole
is
B
(r)
=
dip
4π r 3 [3(m · r̂) · r̂ − m],
R
with the magnetic moment: m = 21 r × JdV
Boundary conditions:
1 E1⊥ = 2 E2⊥ ,
k
k
E1 = E2 ,
B1⊥ = B2⊥ ,
R
r0 ρ(r0 )d3 r0 =
P
i qi ri .
1 k
1 k
B1 =
B .
µ1
µ2 2
Poynting vector: S = µ1 E × B.
1
Energy density: u = 2 E 2 + 2µ
B2.
1
1
Maxwell stress tensor: Tij = 0 Ei Ej − δij E 2 +
Bi Bj −
2
µ0
−1/2
Speed of light: c = (µ)
.
The electric dipole radiation. The electric field in the wave zone:
1
δij B 2 .
2
µ0
[[p̈ × n] × n].
4πr
µ0
[n × m̈].
The magnetic dipole radiation. The electric field in the wave zone: E =
4πcr
Liénard-Wiechert potentials:
V (r, t) =
1
qc
,
4π0 r̃c − r̃ · v
A(r, t) =
E=
v
V (r, t),
c2
where r̃ is the vector from the retarded position to the field point r and v is the velocity of the charge at the retarded
time.
Lorentz transformation:
x̄ = γ(x − vt),
v
t̄ = γ(t − 2 x),
c
1
γ = p
.
1 − v 2 /c2
Intervals: ds2 = c2 dt2 − dx2 − dy 2 − dz 2 .
eB
Relativistic cyclotron frequency: ωB = mcγ
.
The field tensor:


0 −Ex /c −Ey /c −Ez /c
∂Aν
∂Aµ
0
Bz
−By 
 E /c
Fµν =
−
= x
Ey /c −Bz
0
Bx 
∂xµ
∂xν
Ez /c By
−Bx
0
Transformation of fields:
Ēk = Ek ,
B̄k = Bk ,
Ē⊥ = γ(E⊥ + v × B⊥ ),
1
B̄⊥ = γ(B⊥ − 2 v × E⊥ ).
c
Energy momentum four vector: P = mcγ(1, v/c).
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