George Stein

Computational Cosmology

Visualization of a Peak Patch simulation
Containing 60 million dark matter halos.
Visualization by George Stein
Simulation by Alvarez, Bond, Stein

About Me

I am a fourth year PhD student in the Department of Astronomy & Astrophysics at the University of Toronto. I work at the Canadian Institute for Theoretical Astrophysics (CITA) with my thesis supervisor Dick Bond.

My work focuses on understanding the large scale structure of the universe as it evolves from the big bang 13.7 billion years ago until the present day. I work mainly on developing supercomputer simulations which are based on our current understanding of the cosmos, in order to create testable predictions of this cosmic evolution. These simulations are very useful for many cosmological experiments that I am involved in, such as the Atacama Cosmology Telescope, Euclid, COMAP, and the Simons Observatory

This field, sometimes called computational cosmology, combines fundamental physics knowledge with state-of-the art computing power. These type of simulations are extremely useful in the analysis of experimental data & in the design of future telescopes, and as such there is much interest in creating them.

Some groups, such as my friends in the FIRE Collaboration, are attempting to simulate individual galaxies as accurately as possible, by including extremely detailed physics of the inner-workings of galaxies. Even though computers are becoming evermore powerful, these variety of simulations are much too computationally expensive to simulate very large regions of the universe, so for these type of problems we need something else...

In comes my main research project - the development of a very fast way to simulate massive regions of the universe. Called the "peak patch" method, it allows for the creation of thousands of "mock universes" each with over 10's of millions of galaxies, a computational feat hard to match in any other way. Although each galaxy is not as detailed in our simulations as those in something like the FIRE project, we add in a mix of observational data and results from detailed single galaxy simulations to create very accurate mock maps of the sky. The video above is a visualization I created of "flying through" one of our universes!

I have also worked on GPU computing, developing and optimizing algorithms to potentially find fast radio bursts using the CHIME radio telescope, which is underway in Penticton, BC.

Download my CV

if you are curious as to what I have been up to

CV download

Links to my work

Here are some of my talks & posters, movies, and my public data

Talks Posters Movies Data

Contact George

To find out more please feel free to email me.

gstein@cita.utoronto.ca

Or drop by McLennan Physical Laboratories, Room 1405