338 Appendix
∇ζ
′
+
=−
c
ζ
2
+
∇ζ+,
∇
2
ζ
′
+=−
c
ζ
2
+
[
∇
2
ζ+−
2
ζ+
(∇ζ+)
2
]
.
Hence,
1
2
(ζ
′
+
+ζ
′
−
)∇
2
ζ
′
+
−(∇
2
ζ
′
+
)
2
=−
c
2
ζ
3
+
ζ−
[
1
2
(ζ++ζ−)∇
2
ζ+−(∇ζ+)
2
]
=0.
This identity remains valid whenζ
′
+andζ
′
−are interchanged, which proves
the validity of transformationγ. It follows from the particular case in which
c= 1 andd= 0 that if the pairP(φ, ψ) is a solution of (A.12.4) and (A.12.5)
and
φ
′
=
φ
φ
2
+ψ
2
,
ψ
′
=−
ψ
φ
2
+ψ
2
,
then the pairP
′
(φ
′
,ψ
′
) is also a solution of (A.12.4) and (A.12.5). This
relation is applied in Section 6.10.2 on the intermediate solution of the
Einstein equations.
Transformationε
Combining transformationγandδwitha=d= 1 andc=− 2 b, it is found
that ifζ+andζ−are solutions of (A.12.1) and
ζ
′
+=
ζ−−b
ζ−+b
,
ζ
′
−=
b+ζ+
b−ζ+
,
thenζ
′
- andζ
′
−
are also solutions of (A.12.1). This transformation is ap-
plied in Section 6.10.4 on physically significant solutions of the Einstein
equations.
The following formulas are well known and will be applied later. (ρ, z)
are cylindrical polar coordinates:
∇V=
(
∂V
∂ρ
,
∂V
∂z
)
, (A.12.6)
∇·F=
1
ρ
∂
∂ρ
(ρFρ)+
∂Fz
∂z
, (A.12.7)
∇
2
V=
∂
2
V
∂ρ
2
+
1
ρ
∂V
∂ρ
+
∂
2
V
∂z
2