Gravitational Lens, 8C20.40

Topic and Concept:

• General Relativity

Location:

• Cabinet: Optics (OP)

• Bay: (A1)

• Shelf: #1

Abstract:

Lens machined from PMMA (a.k.a. Lucite, Plexiglass, Perspex, etc; n=1.495) as per calculations in C. Darwin, "The Gravity Field of a Particle", Proc. Roy. Soc. A 249, 180 (1959), especially section 8, culminating in equation 29, which gives the deviation of the ray as a function of perihelion distance; see J. Higbie, "Gravitational Lens", Am. J. Phys 49, 652 (1981) for practical details.

Looking through the lens from a viewpoint on the lens axis with the flat side facing the viewer, the lens causes incoming light rays to deviate by same amount as would be caused by a black hole with mass m=2.595 x 10^24 kg (a little less than half the mass of the Earth).

This mass was chosen in order that light with an impact parameter of 1 cm would be captured into the "light ring".

The radius of the light ring would be 0.5774 cm.

The event horizon of such a black hole would have a radius of 0.3849 cm.

Lens made by Sara Yaeger of the UW Physics Dept. Instrument Shop in 2007 using a lathe (from a profile calculated by Jim Reardon based on the above papers).

Setup and Procedure:

The lens can be used to observe Einstein Rings (see photo below).

Of note is that partial Einstein rings may be observed even if the observer, lens and source are only very roughly coaxial--alignment does not need to be perfect.

Discussion:

The best current example of an actual Einstein ring is that caused by the luminous red galaxy LRG 3-757.

Videos:

• Lecture Demonstration's Youtube Channel

References:

• List any references

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