338 Appendix
∇ζ′
+=−
cζ
2
+∇ζ+,∇
2
ζ′
+=−cζ2
+[
∇
2
ζ+−2
ζ+(∇ζ+)2]
.
Hence,
1
2(ζ′
+
+ζ′
−)∇
2
ζ′
+−(∇
2
ζ′
+)
2
=−c
2ζ
3
+
ζ−[
1
2(ζ++ζ−)∇2
ζ+−(∇ζ+)2]
=0.
This identity remains valid whenζ
′
+andζ′
−are interchanged, which provesthe 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′
=φφ
2
+ψ
2,
ψ′
=−ψφ
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−−bζ−+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