Computational Astrophysics
Group information
We study the cosmos through numerical simulations and computational modeling. Our research spans multiple physical scales, addressing key questions in:
- Cosmology: exploring the large-scale structure of the universe, dark matter, and the formation and evolution of galaxies.
- Galactic Dynamics and Structure: investigating the formation and evolution of galaxies, their rotation curves, star formation, and stellar feedback.
- Interstellar Medium (ISM) and Molecular Clouds: modeling the turbulent, magnetized gas that gives birth to stars, including the role of gravity, magnetic fields, and stellar feedback.
- Star Formation: studying the gravitational collapse of dense cores within molecular clouds, fragmentation processes, and accretion phenomena.
- Protoplanetary Discs: simulating the dynamics and evolution of discs around young stars, including planet-disk interactions, migration, and disc fragmentation.
To tackle these complex, multi-scale problems, we employ a suite of advanced numerical tools, including AREPO, FLASH, Gadget, FARGO3D, and Torch. These codes allow us to simulate hydrodynamics, magnetohydrodynamics, gravity, and radiation with high resolution and physical realism.
As a group, we are committed to contribute actively to the international scientific community. Through collaboration and rigorous numerical experimentation, we aim to study the complex physical processes that shape our universe.
Welcome to our webpage, where the wonders of the universe come alive through the power of computation!
