Dark Matter group at the Institute for Astroparticle Physics (IAP)
The Dark Matter Group is conducting research at the Karlsruhe Institute of Technology (KIT) to unravel the nature of "dark matter", one of the greatest mysteries in the Universe. Although Dark Matter manifests itself in many astrophysical and cosmological observations, its particle nature remains unknown so far. Due to the required properties as Dark Matter particle, none of the elementary particles constituting the "Standard Model of Particle Physics" (SM) can make up Dark Matter. Thus, physics beyond the SM is needed. There are many theoretical extensions of the SM giving rise to DM candidates such as the axion or a sterile neutrino. Another model called supersymmetry could naturally contain a lightest supersymmetric particle (LSP) as DM candidate being the so-called weakly interacting massive particle (WIMP).
A promising method for the discovery of WIMPs is the search for scattering processes of WIMPs from the galactic halo scattering off an atomic nucleus of known matter. Such scattering processes are expected to be extremely rare leaving only tiny signatures. To search for such signals requires highly sensitive detectors as much as possible shielded against ambient and cosmic-induced background. There are searches ongoing worldwide with sophisticated technologies and ever more sensitive measuring methods.
We are conducting intensive research and development (R&D) for the current search for dark matter as well as for the next generation of experiments. The Dark Matter Group at the IAP of KIT is a member of the XENON Collaboration (since 2019) and participates in the construction of the XENONnT experiment. Since 2018, we are involved in the development of the follow-up experiment DARWIN. From 2005 to 2020, we have significantly contributed to the setup, operation and data analysis of the EDELWEISS experiment.
The XENON collaboration comprises 163 scientists from 28 institutions across 11 countries. Five German institutions are significantly involved: The Max Planck Institute for Nuclear Physics in Heidelberg, the Universities of Münster, Mainz and Freiburg as well as the Karlsruhe Institute of Technology. The XENON1T experiment running from 2016 to 2018 is being upgraded to its next phase, XENONnT, with an active xenon mass three times larger and a background that is expected to be lower by a factor 6, thus improving even further the world-record sensitivity of XENON1T. XENONnT is expected to start commissioning in 2020. The KIT group is involved in the setup of XENONnT and in the upcoming data analysis.More about XENON
DARk matter WImp search with liquid xenoN (DARWIN) is a future experiment for the direct detection of dark matter based on a multi-ton liquid xenon time projection chamber. DARWIN is a collaborative project of 29 institutions from 12 countries building on the highly successful dual-phase xenon technology developed and explored in the XENON experiment series (XENON10, XENON100, XENON1T). KIT is a founding member of the DARWIN collaboration. We contribute e.g. to the electrostatic design of the TPC, on the suppression of background and on sensitivity studies for Dark Matter and other searches for physics beyond the Standard Model.More about DARWIN
The EDELWEISS collaboration consists of scientists from 4 countries. The experimental setup is based on array of Germanium bolometers installed in the Frejus road tunnel in the underground laboratory (Laboratoire Souterrain de Modane, LSM), which shields the experiment by 1800m of rock (4850 m.w.e.). The bolometer detectors can detect WIMPs via their elastic scattering off Germanium nuclei and have an excellent background rejection power. In the research group at the Institute for Astroparticle Physics (IAP), the muon veto system was designed, built and operated. Besides the analysis of experimental data, we also provided a new electronic data read-out in cooperation with our partner institute IPE at KIT. The EDELWEISS experiment is concentrating on the search of so-called low mass WIMPs with masses in the GeV range.More about EDELWEISS