Gravitational lensing effect through the Cheshire Cat galaxy cluster (in yellow). This cluster acts like a lens that distorts the light of a galaxy behind it (in blue) into several arc-shaped images, so-called "Einstein rings". The combination of the galaxy cluster in the foreground with the distorted background galaxy results in the image of a smiling face. Image: NASA/ESA

With Einstein on crooked paths

How can gravitational waves deflected by lensing effects be found? Machine learning methods will be used to investigate whether the expected diffraction effects can actually be found in the data from gravitational wave detectors. This could be far more than just another spectacular confirmation of Einstein's theory, but a new method for exploring the universe.

An object behind a glass of water appears distorted because the water deflects the incident rays of light. Such a "lens effect" is also caused by gravitational fields: light moving through the universe is deflected, sometimes creating multiple images of the same object. This gravitational lensing effect was predicted by Einstein and has since become an important tool in astrophysics. Gravitational lensing has numerous applications, e.g. in the search for extrasolar planets, the interpretation of images of supermassive black holes or the mapping of the distribution of dark matter.

Gravitational waves: Shaking space and time

Like light, gravitational waves are also deflected and sometimes split into several signals. Einstein predicted these ripples in space-time, which propagate at the speed of light, as early as 1916. In 2015, the first gravitational wave, emitted when two black holes collided in the distant universe, was measured directly. This collective achievement, to which the Max Planck Institute for Gravitational Physics made important contributions, was honored with the Nobel Prize in Physics in 2017. Since then, the emerging field of gravitational wave astronomy has observed 90 confirmed signals and more than 80 significant candidates in the ongoing observational campaign. Machine learning will allow a faster analysis of the rapidly growing data.

Can gravitational waves deflected by lensing effects be found? Miguel Zumalacarregui and his team at the Max Planck Institute for Gravitational Physics have already developed a theory for deflecting gravitational waves and efficient software for calculating these effects. The code delivers precise predictions of complex lens systems in milliseconds.

Research group leader Zumalacarregui wants to use machine learning methods to investigate whether the expected diffraction effects can actually be found in the data from the gravitational wave detectors. The detection of gravitational deflection or its absence will not only provide new insights into gravitational wave astronomy, but will also have profound implications for other areas of astrophysics and fundamental physics, such as the study of the properties of dark matter. Gravitationally deflected gravitational waves could thus be far more than just another spectacular confirmation of Einstein's theory, namely a new method for exploring the universe.

Please support the project with your donation. This will enable us to carry out a research project for which there are currently no funds available.

Go to Editor View