The student will model the gamma-ray emission around the Milky Way's central bubble.

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 focus of this PhD research is the study of the early evolution of life using abundances of chemical elements in different life forms and their environments, at different temporal and spatial scales.

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?