Gravitational Lensing Derivations - Is There Another Way?

In summary, the light's time delation is induced by the "refraction index" n (Saphiro delay) and is related to the gravitational time dilation.
  • #1
ChrisVer
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Hey,
I just had the chance to extract the gravitational lensing caused by a massive point using Fermat's principle.

I was wondering though, is there any other way to do that?

Also is the light's time delation induced by the "refraction index" [itex]n[/itex] (Saphiro delay) connected to "gravitational time delation"?
 
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  • #2
ChrisVer said:
Hey,
[..] gravitational lensing caused by a massive point using Fermat's principle [..]
Also is the light's time delation induced by the "refraction index" [itex]n[/itex] (Saphiro delay) connected to "gravitational time delation"?
Answering your second question: yes indeed, although a bit indirectly. Fermat's principle is related to Huygen's principle and gravitational time dilation follows from the reduced speed of light, which plays a role in calculating the bending of light by that means - see p.821 (and for context p.820) here:
https://en.wikisource.org/wiki/The_...Perihelion-motion_of_the_paths_of_the_Planets.

PS Jonathan Scott provided fitting commentary to that link about the "double bending" here: https://www.physicsforums.com/threads/bending-of-light.787335/#post-4944166
 
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  • #3
As to alternative derivations, it is worth noting the Hugen's and Fermat's principle are derived results in GR, even more so than the geodesic principle (which can be derived from the field equations, so it need not be assumed separately). Einstein used this principle in his derivations without proof (so far as I know) - he assumed it must be true based physical intuition. (Pauli, in his 1921 work, provides a justification for this based on work by Levi-Civita and Weyl; at that time, it was only proved for spherical symmetry, and unknown whether such a principle had any validity in a more general spacetime. MTW justifies Fermat's principle for any static solution).

Most modern books derive lensing directly treating null geodesic paths, without bothering to use (let alone justify) Huygen's principle or Fermat's principle and a varying speed of light (which is coordinate dependent). For example the following all use pure null geodesic analysis for light bending with no mention at all of Huygen's or Fermat's principle or varying light speed:

P. G. Bergmann's 1942 text (enthusiastically endorsed by Einstein)
J.L. Synge 1960 General Relativity book
James L. Anderson's 1967 Principles of Relativity Physics

Misner, Thorne, & Wheeler derive light bending directly from null geodesic analysis, but for Shapiro time delay they introduce and justify Fermat's principle for static fields, and imply it isn't true [or even definable] in more general cases.
 
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1. What is gravitational lensing and why is it important?

Gravitational lensing is a phenomenon in which the gravitational pull of a massive object bends and distorts the light from objects behind it. It is important because it allows us to study and observe distant objects that would otherwise be too faint or small to see. It also helps us understand the distribution of matter in the universe.

2. How is gravitational lensing typically studied and measured?

Gravitational lensing is mainly studied through observations of the distorted light from distant objects, such as galaxies or quasars, behind a massive object. This can be done using telescopes and other instruments that can detect and measure the bending of light. The amount of distortion can also be measured and used to calculate the mass and properties of the lensing object.

3. What are some common techniques used for deriving gravitational lensing equations?

One common technique used for deriving gravitational lensing equations is through the use of the equations of general relativity, which describe the relationship between mass, energy, and the curvature of space-time. Other techniques include using geometric optics and ray tracing methods, as well as numerical simulations and observations of lensing events.

4. Is there another way to derive gravitational lensing equations besides using general relativity?

While general relativity is the most commonly used framework for deriving gravitational lensing equations, there are other alternative theories of gravity that can also be used, such as modified Newtonian dynamics (MOND) and scalar-tensor theories. These alternative theories may provide different predictions and can be tested through observations of gravitational lensing events.

5. How is gravitational lensing used in practical applications?

Gravitational lensing has several practical applications in astronomy and cosmology. It can be used to study the properties and distribution of dark matter, as well as to measure the expansion rate of the universe. It can also be used to detect and study exoplanets, as well as to map the cosmic web of large-scale structures in the universe. In addition, gravitational lensing has potential applications in technologies such as gravitational wave detectors and space-based telescopes.

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