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Dark UNiverse Explorations

Tim Schrabback (ORCID: 0000-0002-6987-7834)
  • Grant DOI 10.55776/F101300
  • Funding program Special Research Areas
  • Status Ongoing
  • Start March 1, 2026
  • End February 28, 2030
  • Funding amount € 3,249,922

Disciplines

Physics, Astronomy (100%)

Keywords

  • Cosmology,
  • Galaxy clusters,
  • Dwarf galaxies,
  • Cosmological simulations,
  • Euclid,
  • JWST
Abstract

The new Special Research Area (SFB) Dark UNiverse Explorations (DUNE) of the Austrian Science Fund (FWF) is a collaboration between researchers from the Universities of Innsbruck and Vienna, as well as the Institute of Science and Technology Austria (ISTA). One of DUNE`s central goals is to learn more about dark matter and dark energy in the Universe. Together, these invisible components make up 95% of the Universe`s energy content, yet their respective physical nature remains largely unknown. Neither dark matter nor dark energy can be observed directly. Indirectly, however, they leave signatures, for example, in the distributions and properties of galaxies, in the number density of massive galaxy clusters, and in coherent distortions of the observed galaxy shapes caused by gravitational lensing. Comparing galaxy observations with theoretical models can therefore shed light on the dark components of the Universe. DUNE uses observational data from two new space telescopes: The European Space Agency`s (ESAs) Euclid mission was launched in July 2023 and is expected to deliver high-resolution images of more than a third of the night sky by the end of the decade. The James Webb Space Telescope (JWST), a joint project of NASA, ESA, and the Canadian Space Agency (CSA), allows scientists to peer deep into the past of the Universe in small regions of the sky. As part of international research collaborations, the DUNE team analyzes Euclid data at the University of Innsbruck and observational data from the JWST at the ISTA. To draw conclusions about the properties of dark matter and dark energy, the observational results are compared with simulated "virtual universes". These simulations are (co-)developed at the University of Vienna and model cosmic structure formation in these digital reconstructions of our universe: COLIBRE is a simulation project that includes a small number of highly detailed simulations. Complementary to this are the simulations from the DISCO-DJ project, which can quickly make predictions for many different theories and utilize the new Austrian supercomputer MUSICA. DUNE opens a new window to the dark Universe for Austria and brings us one step closer to answering some of the biggest questions in modern cosmology. Links: - COLIBRE: www.colibre-simulations.org - Euclid: https://www.euclid-ec.org/ , https://www.esa.int/Science_Exploration/Space_Science/Euclid - JWST: https://esawebb.org/, https://science.nasa.gov/mission/webb/ - DISCO-DJ: https://cosmology.univie.ac.at, https://arxiv.org/abs/2510.

Consortium
  • Francine Marleau, Universität Innsbruck
    consortium member (01.03.2026 -)
  • Jorryt Matthee, Institute of Science and Technology Austria - ISTA
    consortium member (01.03.2026 -)
  • Laila Linke, Universität Innsbruck
    consortium member (01.03.2026 -)
  • Oliver Hahn, Universität Wien
    consortium member (01.03.2026 -)
  • Sebastian Grandis, Universität Innsbruck
    consortium member (01.03.2026 -)
  • Sylvia Ploeckinger, Universität Wien
    consortium member (01.03.2026 -)
  • Tim Schrabback, Universität Innsbruck
    consortium member (01.03.2026 -)
Research institution(s)
  • Universität Innsbruck
Project participants
  • Florian List, Universität Wien , national collaboration partner
International project participants
  • Yannick Mellier, Observatoire de Paris - France
  • Bocquet Sebastian, Ludwig Maximilians-Universität München - Germany
  • Angus Wright, Ruhr-Universität Bochum - Germany
  • Joop Schaye, Universiteit Leiden - Netherlands
  • Matthieu Schaller, Universiteit Leiden - Netherlands
  • Angulo Raul, University of the Basque Country - Spain
  • William G. Hartley, University of Geneva - Switzerland
  • Julian Adamek, University of Zurich - Switzerland
  • Bleem Lindsey, Argonne National Laboratory - USA
  • Carlos Frenk, Durham University

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