The ISM of spiral galaxies is a dynamic environment consisting of thermal gas, relativistic particles, magnetic fields, and dust. The project aims to decipher the origin of filamentary structures in the ISM using numerical simulations as well as observational data.

This project delves deep into understanding how stars create elements, contributing to unraveling the mysteries surrounding the origins of elements by extracting and tracing the element compositions of millions of stars using cutting-edge spectroscopic surveys.

Supermassive black holes in the early Universe are more massive than we can presently explain. We aim to construct their demographics and reveal their origin.

The student will work with Prof. Krumholz to design and run simulations using the enzo adaptive mesh refinement code.

By mapping the motions of many galaxies, this project aims to precisely measure the amount and distribution of both visible and dark matter and test Einstein’s theory of gravity.

By mapping the motions of many galaxies, this project aims to precisely measure the amount and distribution of both visible and dark matter and test Einstein’s theory of gravity.

The goal of this project is to use new, high-resolution simulations to understand how key physical processes, like stellar feedback and gravitational instabilities, shape disk galaxies (from 11 Gyr ago to today).

In this project you will use a new cosmic ray propagation code, CRIPTIC, to model the injection, transport, and final annihilation of positrons in the interstellar medium of the inner Galaxy.

In this project you will use a new cosmic ray propagation code, CRIPTIC, to model the injection, transport, and final annihilation of positrons in the interstellar medium of the inner Galaxy.

We aim to build a novel framework to study supermassive black holes via their unique gravitational wave signatures providing a multi-messenger tool to constrain galaxy formation in the early universe.

In this project you will use some combination of theoretical population synthesis calculations and/or analysis of public data from the Fermi telescope to examine the question: what is the real origin of the Galactic Centre Gamma-Ray Excess?

In this project you will use some combination of theoretical population synthesis calculations and/or analysis of public data from the Fermi telescope to examine the question: what is the real origin of the Galactic Centre Gamma-Ray Excess?