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You can find more information about gravitational lensing
and a short introductory lecture in the text of
Peter
D.
Ochsner: Gravitational
Lensing. A sourcebook of applications
and new technology. Springer
-Verlag, New York-Heidelberg-Berlin,
2010.
This book also introduces gravitational lensing
in more details and in mathematical language.
Since the original formulation of
the theory, lots of new advances in the
field have been made.
However, Einstein’s formulation was
the first theoretical attempt to
understand the mechanism behind this
phenomenon, and it is still useful today
to describe this and other effects.
There are many new effects of gravitational lensing that are being
discovered in astronomy.
Here I show you some of these new effects
with my own examples.
The theory of the simplest type of gravitational lensing is the simplest
class of lensing. It is called as “regular lensing”.
In this type of lensing, two or more
objects (e.g. galaxies) are at a fixed distance
from each other. This means that
the distances between each object and
the observer are fixed.
In a binary lens system, the mass of
both lens objects contribute to gravitational
lensing. However, if the distance between
the lens objects is very large, it is not
important for gravitational lensing whether
or not there is a mass in between them.
The position of the source is at fixed
distance from both lens objects.
Therefore, the distance between each
image and the observer is also fixed.
This means that one image is formed at
each image of the source.
The images of the source are arranged
one after the other.
The separation of the images is determined
by the angle between the source and the
lens objects.
The light is bent by the gravitational
field of the two lens objects. This bending
is smallest for the light passing
straight through the center between
the lens objects.
Therefore, the images closest to the
center are called the Einstein Cross.
As a result of the bending of light, the
brightness and size of the images are affected.
In regular lensing, the size of the
images is much smaller than the size of the
source.
The lensing objects have to be located eea19f52d2

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