Research Areas

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.