An Optical Demonstration of Gravitational Lensing

Samantha Scibelli and John Noé
Laser Teaching Center
Stony Brook University

Einstein’s theory of general relativity revolutionized modern physics in the early 1900s by identifying gravity as a geometric property of space and time, known as space-time; it follows that massive objects can distort this space-time. Einstein's theory was confirmed by observations during a solar eclipse in 1919. Today many other experimental observations, such as gravitational waves, gravitational redshift, gravitational time delay and gravitational lensing, have further confirmed Einstein’s predictions. Gravitational lensing can be defined simply as the focusing of light from distant stars or galaxies when the closer intervening object, or 'lens', is massive enough. It was not until 1979 that astronomers actually saw evidence of these gravitational lenses [1]. If this lens is massive enough multiple images of the light source can be produced, by what is known as strong lensing. Otherwise, sometimes the image will only be distorted, in what is referred to as weak lensing. The amount of magnification and distortion will depend on the properties of the lens as well as the relative distances of the observer, source, and galaxy. While gravitational lensing is best seen over the large scale of the universe, we can also create optical experiments in the laboratory that show the same effects.

In this project we are investigating a variety of ways to optically demonstrate and simulate gravitational lensing. It turns out that the base of a wine glass is the perfect shape to demonstrate this lensing effect [2]. (We can use the inferred mass distribution from a galaxy size mass lens to derive the corresponding refractive index distribution. A piece of glass with the appropriate shape can demonstrate the same lensing effect seen with galaxies and galaxy clusters.) We have observed this lensing effect when the base of a wine glass was held up to a concentrated light source, in our case a small LED light. Under suitable circumstances, a very strong gravitational lensing effect was seen where a continuous image of the light source could be seen in a ring shaped pattern (Einstein Ring) around the circular base of the wine glass. We hope to describe these images by optical lens equations and model them in a computer program [3].