Developing galaxy formation models for large-scale cosmological simulations.
Simulating dwarf galaxies to test the nature of dark matter.
Exploring the strength and topology of large-scale magnetic fields.
Studying the impact of anisotropic thermal conduction with the intracluster medium.
Developing new methods to incorperate dust physics in galaxy formation simulations.
Solving small-scale problems of LCDM with alternative dark matter models.
Making predictions for dark matter detection experiments.
Resolving the fine-grained phase-space structure of dark matter.