Research Fields at MPA
The MPA is the major German institution dedicated to theoretical and interpretational research in astrophysics and cosmology. Areas of interest include stellar astrophysics, computational astrophysics and cosmology, the structure, evolution and clustering of galaxies, cosmic large-scale structure, gravitational lensing, microwave background studies and physical cosmology. Because of the close cooperation of the various groups and the fact that often the different areas overlap, there is no strict distinction between the individual areas of research at the Institute.
Further information may be found below and by following the links in the menu on the left.
Large-scale computer simulations are the primary research tool for understanding how the complex structure of the universe emerged from the remarkably simple initial conditions seen in microwave background maps. MPA scientists are active in all aspects of such simulations, developing the numerical codes, deploying them on the largest available supercomputers, and using the results to interpret observational data on galaxies, galaxy clusters and the large-scale structure.
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Research in galaxy formation at MPA uses a variety of theoretical techniques, ranging from direct numerical simulations to analytic and semi-analytic modelling. In addition, we are involved in the detailed analysis of large observational surveys. Millennium Simulations Semi-analytic Modelling Hydrodynamical Simulations The Sloan Digital Sky Survey´
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Understanding how stars work is part of understanding our own Cosmic History, since we are made of “stardust”; the oxygen we breathe, the carbon in our muscles and the iron in our blood were once fused inside stars that have now long gone. The stellar department focusses on open research questions that relate to all aspects of how stars work: how they live their lives (alone, in pairs or as multiples), how they die (gently or giving rise to spectacular supernova explosions), as well as the afterlives of their remnants (white dwarves, neutron stars and black holes), which can be probed through Gravitational Waves.
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Research on physical cosmology at MPA tries to understand the physics responsible for the accelerated expansion of our Universe, both at early and late times, using state-of-the-art data and laws of physics.
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High Energy Astrophysics research deals largely with the interaction of matter with radiation under extreme physical conditions.
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