G
,
H
{\displaystyle \mathrm {G,H} }
the components of the rector potential, and
σ
{\displaystyle \sigma }
the specific resistance of the metal.
σ
u
=
−
b
ω
ϵ
i
p
t
−
d
F
d
t
−
d
ψ
d
x
,
σ
v
=
−
a
ω
ϵ
i
p
t
−
d
G
d
t
−
d
ψ
d
y
,
σ
w
=
−
d
H
d
t
−
d
ψ
d
z
;
}
{\displaystyle \left.{\begin{alignedat}{2}\sigma u&=-b\omega \epsilon ^{ipt}&&-{\dfrac {d\mathrm {F} }{dt}}-{\dfrac {d\psi }{dx}},\\\\\sigma v&=-a\omega \epsilon ^{ipt}&&-{\dfrac {d\mathrm {G} }{dt}}-{\dfrac {d\psi }{dy}},\\\\\sigma w&=&&-{\dfrac {d\mathrm {H} }{dt}}-{\dfrac {d\psi }{dz}};\end{alignedat}}\right\}}
(2)
and therefore
−
σ
4
π
μ
′
∇
2
F
=
−
b
ω
ϵ
i
p
t
−
d
F
d
t
−
d
ψ
d
x
,
−
σ
4
π
μ
′
∇
2
G
=
a
ω
ϵ
i
p
t
−
d
G
d
t
−
d
ψ
d
y
,
−
σ
4
π
μ
′
∇
2
H
=
−
d
H
d
t
−
d
ψ
d
z
.
{\displaystyle {\begin{alignedat}{2}-{\dfrac {\sigma }{4\pi \mu '}}\nabla ^{2}\mathrm {F} &=-b\omega \epsilon ^{ipt}&&-{\dfrac {d\mathrm {F} }{dt}}-{\dfrac {d\psi }{dx}},\\\\-{\dfrac {\sigma }{4\pi \mu '}}\nabla ^{2}\mathrm {G} &=a\omega \epsilon ^{ipt}&&-{\dfrac {d\mathrm {G} }{dt}}-{\dfrac {d\psi }{dy}},\\\\-{\dfrac {\sigma }{4\pi \mu '}}\nabla ^{2}\mathrm {H} &=-{\dfrac {d\mathrm {H} }{dt}}&&-{\dfrac {d\psi }{dz}}.\end{alignedat}}}
In the dielectric outside the sphere, if
f
,
g
,
h
{\displaystyle f,g,h}
are the electric displacements,
K
{\displaystyle \mathrm {K} }
the specific inductive capacity, and if
∂
/
∂
t
{\displaystyle \partial /\partial t}
denote partial differentiation with respect to the time, the equations are
4
π
K
f
=
−
d
F
d
t
−
d
ψ
d
x
=
−
(
∂
∂
t
−
ω
ϵ
i
p
t
d
d
z
)
F
−
d
ψ
d
x
,
4
π
K
g
=
−
d
G
d
t
−
d
ψ
d
y
=
−
(
∂
∂
t
−
ω
ϵ
i
p
t
d
d
z
)
G
−
d
ψ
d
y
,
4
π
K
h
=
−
d
H
d
t
−
d
ψ
d
z
=
−
(
∂
∂
t
−
ω
ϵ
i
p
t
d
d
z
)
H
−
d
ψ
d
z
;
{\displaystyle {\begin{array}{l}{\dfrac {4\pi }{\mathrm {K} }}f=-{\dfrac {d\mathrm {F} }{dt}}-{\dfrac {d\psi }{dx}}=-\left({\dfrac {\partial }{\partial t}}-\omega \epsilon ^{ipt}{\dfrac {d}{dz}}\right)\mathrm {F} -{\dfrac {d\psi }{dx}},\\\\{\dfrac {4\pi }{\mathrm {K} }}g=-{\dfrac {d\mathrm {G} }{dt}}-{\dfrac {d\psi }{dy}}=-\left({\dfrac {\partial }{\partial t}}-\omega \epsilon ^{ipt}{\dfrac {d}{dz}}\right)\mathrm {G} -{\dfrac {d\psi }{dy}},\\\\{\dfrac {4\pi }{\mathrm {K} }}h=-{\dfrac {d\mathrm {H} }{dt}}-{\dfrac {d\psi }{dz}}=-\left({\dfrac {\partial }{\partial t}}-\omega \epsilon ^{ipt}{\dfrac {d}{dz}}\right)\mathrm {H} -{\dfrac {d\psi }{dz}};\end{array}}}
and therefore
−
1
μ
K
∇
2
F
=
−
(
∂
∂
t
−
ω
ϵ
i
p
t
d
d
z
)
2
F
−
(
∂
∂
t
−
ω
ϵ
i
p
t
d
d
z
)
d
ψ
d
x
,
{\displaystyle -{\dfrac {1}{\mu K}}\nabla ^{2}\mathrm {F} =-\left({\dfrac {\partial }{\partial t}}-\omega \epsilon ^{ipt}{\dfrac {d}{dz}}\right)^{2}\mathrm {F} -\left({\dfrac {\partial }{\partial t}}-\omega \epsilon ^{ipt}{\dfrac {d}{dz}}\right){\dfrac {d\psi }{dx}},}
(3)
with a similar equation for
G
{\displaystyle \mathrm {G} }
.
From the form of these equations we see that the solution will take the form
ψ
=
ψ
0
+
ψ
1
ϵ
i
p
t
+
ψ
1
′
ϵ
−
i
p
t
+
ψ
2
ϵ
2
i
p
t
+
ψ
2
′
ϵ
−
2
i
p
t
+
…
F
=
F
1
ϵ
i
p
t
+
F
1
′
ϵ
−
i
p
t
+
F
2
ϵ
2
i
p
t
+
F
2
′
ϵ
−
2
i
p
t
.
{\displaystyle {\begin{array}{l}\psi =\psi _{0}+\psi _{1}\epsilon ^{ipt}+\psi '_{1}\epsilon ^{-ipt}+\psi _{2}\epsilon ^{2ipt}+\psi '_{2}\epsilon ^{-2ipt}+\dots \\\\\mathrm {F} =\mathrm {F} _{1}\epsilon ^{ipt}+\mathrm {F} '_{1}\epsilon ^{-ipt}+\mathrm {F} _{2}\epsilon ^{2ipt}+\mathrm {F} '_{2}\epsilon ^{-2ipt}.\end{array}}}
If we substitute these values in the above equations, we see that we may put
ψ
1
′
ψ
2
′
…
F
1
′
,
F
2
′
{\displaystyle \psi '_{1}\ \psi '_{2}\dots \mathrm {F} '_{1},\ \mathrm {F} '_{2}}
all equal to zero.
If
e
{\displaystyle e}
is the quantity of electricity on the sphere,
ψ
0
=
e
K
r
.
{\displaystyle \psi _{0}={\dfrac {e}{\mathrm {K} r}}.}