Mapping dark matter in galaxy clusters to constrain dark energy
In the last years, observations have shown that the expansion of the Universe is accelerating, despite all the massive galaxies in it attracting each other gravitationally. The reason for this acceleration is unknown; it may be related to a missing link in fundamental physics (the "problem" of Einstein's cosmological constant). Currently, the best way to study the nature of this "dark energy" component is through astronomical observations. Large efforts are being undertaken presently across many countries for this study. One method uses the evolution with time of the most massive clearly defined structures in the Universe: galaxy clusters. With the ultimate goal of helping constrain this evolution, the master's thesis work would concentrate on reduction and analysis of, mostly, X-ray data of galaxy clusters.
The research group is also involved in the new eROSITA X-ray space telescope, launched in 2019. eROSITA will lead X-ray cluster survey science world-wide for many years to come. Furthermore, we're working towards the ESA Large Mission Athena. The exact master's thesis topic can be adjusted to best fit the interests of the student. Just stop by (office 2.017, Thomas Reiprich) and we can discuss. Note that it is a significant advantage if you have passed well at least one of the following lectures: Radio and X-ray Observations of Dark Matter and Dark Energy (WS), Multiwavelength Observations of Galaxy Clusters (SS), X-ray Astronomy (SS).