Theoretical astrophysicists utilize mathematical or numerical models to probe the astrophysical processes to provide insight into the today's most important problems and place observations into context. 

Research Highlights

Gamma Ray image of the LMC
Gamma ray image of the LMC from Foreman et al. 2015.

High-Energy Messengers: Cosmic Rays, Gamma Rays, and Neutrinos

The most violent environments in the cosmos give rise to the most energetic particles in nature.  Illinois theorists use the highest energy photons (gamma rays), protons and nuclei (cosmic rays), and ghostly neutrinos, together to probe physics at the extremes--from supernova explosions to supermassive black hole jets to galaxy clusters.  In turn, the interactions of these particles with their environments determine the conditions for star and planet formation, and for the evolution of interstellar matter and galaxy evolution.

Links to research groups and facilities: Charles GammieBrian FieldsPaul Ricker

Simulation of a disk around a black hole.
Black hole in the center, left shows the material in the disk while the right shows the radiation energy component  in the disk

General relativistic radiation magnetohydrodynamics : Black Hole Accretion

Many faculty utilize magnetohydrodynamics to understand physical systems.  For example, the temperatures of disks around slowly accreting black holes are set by the balance of turbulent heating, advection, and radiative cooling. In particular, Compton scattering globally couples the disk thermodynamics through the radiative transfer equation. To model these systems, we have developed a numerical method for frequency-dependent general relativistic radiation magnetohydrodynamics (GRRMHD) with Monte Carlo transport. The simulation pictured was performed on the stampede2 supercomputer, an NSF-supported XSEDE resource.

Links to research groups and facilities: Charles Gammie, XSEDE

N-Body Simulations: Dark matter in distant galaxies

Gravitational Lensing Technique
Probing the structure of the Universe by gravitational lensing

Despite decades of study, the nature of dark matter in the universe remains unknown. A new route to exploring its properties is to study the fine-scale structure of the gravitational potentials of distant galaxies. Researchers at Illinois are working on all aspects of this problem: developing new models for dark matter, running massively parallel N-body simulations to determine the resulting fine-scale structure for these new models, and developing new algorithms for analysis of the large observational data sets.

Links to research groups and facilities: Gil Holder, XSEDE, Blue Waters


Faculty Interested in Theory

Name Research Interests
Physics of Inflation in the Early Universe ; Connections Between High-Energy Particle Physics and the Early Universe
Cosmology, Nuclear and Particle Astrophysics; Nucleosynthesis; Dark Matter; Cosmic-ray, Gamma-ray, and Neutrino Astrophysics; Supernovae; Astrobiology
Black Holes; Formation of the Moon; Planet Formation; Star Formation; Cosmic-ray Transport; Interstellar Turbulence
Cosmic Microwave Background; Gravitational Lensing; Dark Matter; Dark Energy; Black Holes
Cosmic Magnetic Fields; Formulation of Theory of Star Formation Accounting for Role of Magnetic Fields; Astrophysical Analytical and Numerical Magnetohydrodynamics; Diffuse Matter Astrophysics
Computational Astrophysics; Cosmological Structure Formation; Clusters of Galaxies; Binary Stars; Supernovae
Multimessenger Astronomy; Numerical Relativity; Gravitational Waves; Scientific Computing; Data Science
General Relativity; Numerical Relativity; Gravitational Wave Astrophysics; Computational Magnetohydrodynamics and Stellar Dynamics; Cosmology
Dark Matter; Particle Astrophysics; Particle Physics of the Early Universe