Multiple images in gravitational lensing

In summary, the conversation discussed the concept of multiple images in weak lensing. The proper time delay and Fermat's principle were mentioned as determining factors for the formation of multiple images at critical points, such as maxima and saddle points. It was also noted that each maximum or saddle point can create two distinct images with varying brightness and orientation.
  • #1
Angelos K
48
0
Dear all,

so far I have only studied weak lensing. Therefore I understand little about multiple images.The light paths, by Fermat's principle, have to correspond to stationary points of the (proper) time delay. Minima, maxima saddle points. Basics are nicely reviewed here [p.14]:
http://www.ita.uni-heidelberg.de/research/bartelmann/Lectures/EinfSeminar/JeruLect.pdf

My question is why saddle points and maxima correspond to multiple images as for example claimed here [p.11]:
Takahashi et al. 2011
Am I right to assume that each maximum or saddle point creates two images?

All the best,
Angelos
 
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  • #2
Yes, you are right to assume that each maximum or saddle point creates two images. This is because the light paths of multiple images must converge at the critical points (maxima and saddle points). The saddle points correspond to two distinct images that have different brightness and orientation, whereas maxima correspond to two identical images that have the same brightness and orientation. Therefore, multiple images can be formed when light passes through a critical point such as a maximum or saddle point.
 

1. What is gravitational lensing?

Gravitational lensing is a phenomenon in which the light from a distant object is bent by the gravitational field of a massive object, such as a galaxy or a cluster of galaxies, in its path. This results in the formation of multiple images of the same object, distorted and magnified in different ways.

2. How does gravitational lensing produce multiple images?

When light from a distant object passes through the gravitational field of a massive object, it follows the curvature of space-time and gets bent. If the alignment is just right, the light can be bent in such a way that we see multiple images of the same object. This is similar to how a magnifying glass bends and focuses light to produce a larger image.

3. What are the different types of gravitational lensing?

There are two main types of gravitational lensing: strong lensing and weak lensing. Strong lensing occurs when the light is significantly distorted, resulting in highly magnified and multiple images of the same object. Weak lensing, on the other hand, produces subtle distortions in the shape of the background object, making it appear stretched or sheared.

4. How do scientists use multiple images in gravitational lensing to study distant objects?

By studying the different images produced by gravitational lensing, scientists can gather information about the properties of the lensing object, such as its mass and distribution. They can also use the lensing effect to magnify and study distant galaxies and other objects that would otherwise be too faint to detect.

5. Can gravitational lensing be used to test Einstein's theory of general relativity?

Yes, gravitational lensing is one of the key pieces of evidence supporting Einstein's theory of general relativity. The bending of light by massive objects is a direct consequence of the theory, and the precise measurements of multiple images in gravitational lensing have confirmed its predictions.

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