General Info
Primary Interests: Cosmology, Black Holes, and also Planetary Astrophysics
Actual Research: Modeling Black Hole Growth History, Effects of Modified Gravity on Power Spectra Through its Impact on Large Scale Structure Evolution
Supervisor: Dr. Rachel Bean
And for the sake of having some pictures:
A small subsection of the simulation results for the formation of large scale structure presented as the result of a simulation from z=50 to z=0 (today). Each side of the box shown is 20 Mpc /h in size and the box represents 8/1000 of the simulation volume, and includes 8,490 of the 1283 (=2,097,152) total particles. The simulation is carried out for standard gravity, and is obtained via use of A. Klypin's Particle Mesh code.
Two screenshots from a program I wrote using OpenGL and C++ to create accurate renderings of Mars' Moons. (Phobos is depicted).