Help Deriving formula for Einstein Radius

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SUMMARY

The Einstein ring radius, denoted as R_e, is defined by the formula R_e = 2[GMx(L-x)/(Lc^2)]^1/2, where G is the gravitational constant, M is the lens mass, L is the distance to the source, and x is the distance to the lens mass. To derive this formula, one must utilize the light bending formula for small angles, specifically delta_phi = 4GM/(bc^2), and apply Euclidean geometry principles. The alignment of the source, lens, and observer is crucial, as indicated by setting \theta_S = 0 for the Einstein ring configuration.

PREREQUISITES
  • Understanding of gravitational lensing concepts
  • Familiarity with the light bending formula for small angles
  • Basic knowledge of Euclidean geometry
  • Proficiency in manipulating algebraic formulas
NEXT STEPS
  • Study the derivation of the Einstein ring formula in detail
  • Learn about gravitational lensing and its applications in astrophysics
  • Explore the implications of light bending in general relativity
  • Investigate the geometry involved in lensing scenarios
USEFUL FOR

Astronomers, physicists, and students studying gravitational lensing and general relativity will benefit from this discussion, particularly those interested in the mathematical derivation of the Einstein ring radius.

adwbizi1
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I have been trying to show that the Einstein ring radius R_e = 2[GMx(L-x)/(Lc^2)]^1/2
to no avail. can someone who knows this show me, or at least point out the direction. I have a strong hunch that i'll have to use the light bending formula for small angles 
delta_phi = 4GM/(bc^2), and geometry.

The Einstein radius is the radius of the ring image formed when a bright source is exactly behind a spherically symmetric lens mass. L is the distance to the source, and x is the distance to the lens mass.
 
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adwbizi1 said:
I have been trying to show that the Einstein ring radius R_e = 2[GMx(L-x)/(Lc^2)]^1/2
to no avail. can someone who knows this show me, or at least point out the direction. I have a strong hunch that i'll have to use the light bending formula for small angles
delta_phi = 4GM/(bc^2), and geometry.

The Einstein radius is the radius of the ring image formed when a bright source is exactly behind a spherically symmetric lens mass. L is the distance to the source, and x is the distance to the lens mass.

The formula on http://en.wikipedia.org/wiki/Einstein_ring" can be derived using the light bending formula for small angles. Also, assume Euclidean geometry and use \theta \doteq \sin\theta \doteq \tan\theta. Click on the diagram, and take \theta_S = 0, since, for an Einstein ring, the source, lens, and observer have to be lined up.

If you need more help, just ask.
 
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