386 Gravitational lensing
is thedeflection potential, which does not depend onη. The Fermat principle can
thus be written as dt/dξ =0, and inserting equation (14.19) one once again
obtains the lens equation
η=
Ds
Dd
ξ−Ddsα(ξ), (14.22)
whereαis defined in equation (14.10). (If we defineβ=η/Dsandθ=ξ/Dd
we obtain equation (14.13). One can also write equation (14.22) as follows.
∇ξ(ˆ ξ,η)= 0 , (14.23)
which is an equivalent formulation of the Fermat principle.
The arrival time delay of light rays coming from two different images (due
to the same source inη) located inξ(^1 )andξ(^2 )is given by
c(t 1 −t 2 )=(ˆ ξ(^1 ),η)−(ˆ ξ(^2 ),η). (14.24)
14.2.4 Remarks on the lens equation
It is often convenient to write (14.22) in a dimensionless form. Letξ 0 be a length
parameter in the lens plane (whose choice will depend on the specific problem)
and letη 0 =(Ds/Dd)ξ 0 be the corresponding length in the source plane. We set
x=ξ/ξ 0 ,y=η/η 0 and
κ(x)=
&(ξ 0 x)
&cr
, α(x)=
DdDds
ξ 0 Ds
αˆ(ξ 0 x), (14.25)
where we have defined a critical surface mass density
&cr=
c^2
4 πG
Ds
DdDds
= 0 .35 g cm−^2
(
1Gpc
D
)
(14.26)
withD≡DdDDsds(1 Gpc= 109 pc). Then equation (14.22) reads as follows
y=x−α(x), (14.27)
with
α(x)=
1
π
∫
R^2
x−x′
|x−x′|^2
κ(x′)d^2 x′. (14.28)
In the following we will mainly use the previous notation rather than that in
equation (14.28).
An interesting case is a lens with a constant surface mass density&. With
equation (14.11) one then finds, for the deflection angle,
α(θ)=
4 G
c^2 ξ
&πξ^2 =
4 πG&
c^2
Ddθ, (14.29)