To understand how our galaxy, the Milky Way, came to be how it is today, we need to understand how galaxies, in general, change and interact with their environment. However, it is currently challenging to observe the environment around galaxies. This thesis investigates using a new type of radio probe, fast radio bursts, to study how galaxies evolve and the low-density material between them. We analysed simulations of the Universe and determined that with the upcoming Square Kilometre Array telescope, we will obtain enough data for fast radio bursts to constrain galaxy evolution.
History
Thesis type
Thesis (PhD)
Thesis note
Presented in fulfilment of the requirements of the degree of Doctor of Philosophy, School of Science, Computing and Engineering Technologies, Swinburne University of Technology, Melbourne, Australia, 2022.