Simulating the universe: the evolution of the most massive galaxies

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dc.contributor.author Rennehan, Douglas
dc.date.accessioned 2022-04-19T16:25:34Z
dc.date.available 2022-04-19T16:25:34Z
dc.date.copyright 2022 en_US
dc.date.issued 2022-04-19
dc.identifier.uri http://hdl.handle.net/1828/13859
dc.description.abstract The cores of galaxy clusters contain the most massive galaxies in the Universe, the brightest cluster galaxies. These galaxies are unique compared to their counterpart galaxies outside of clusters as they have much brighter cores, and vast spatially- extended stellar envelopes. The theoretical picture of how they reached their huge masses relied on the idea of gradual stellar mass growth during the second half of the history of the Universe. However, recent observational evidence of highly-overdense protoclusters, the progenitors of these galaxies, demonstrates that some brightest cluster galaxies may have assembled within the first few billion years after the Big Bang – seemingly contradicting our theoretical predictions. I include my theoretical work that shows the short timescales over which these observed protoclusters trans- form into the brightest cluster galaxies and discuss the likelihood of finding these rare protoclusters in the early Universe. To push our understanding of the rapid evolution of these galaxies even further for- ward demands the use of numerical simulations due to the highly coupled, non-linear astrophysical processes that occur during the process. In this dissertation, I include improvements to our numerical models of hydrodynamical turbulence and supermas- sive black holes that I incorporated into a state-of-the-art hydrodynamical+gravity simulation code, in effort to provide the groundwork to improving our understanding of the build-up of the brightest cluster galaxies in the early Universe, and galaxy evolution in general. en_US
dc.language English eng
dc.language.iso en en_US
dc.rights Available to the World Wide Web en_US
dc.subject hydrodynamics en_US
dc.subject turbulence en_US
dc.subject black holes en_US
dc.subject galaxy evolution en_US
dc.subject numerical simulation en_US
dc.subject brightest cluster galaxy en_US
dc.subject galaxy cluster en_US
dc.title Simulating the universe: the evolution of the most massive galaxies en_US
dc.type Thesis en_US
dc.contributor.supervisor Babul, Arif
dc.degree.department Department of Physics and Astronomy en_US
dc.degree.level Doctor of Philosophy Ph.D. en_US
dc.identifier.bibliographicCitation D. Rennehan. 2021. Mixing matters. MNRAS, 506, 2, pp. 2836–2852. en_US
dc.identifier.bibliographicCitation D. Rennehan, A. Babul, C. C. Hayward, C. Bottrell, M. H. Hani, S. C. Chapman. 2020. Rapid coeval star formation and assembly of the most massive galaxies in the universe. MNRAS, 493, pp. 4607-4621. en_US
dc.identifier.bibliographicCitation D. Rennehan, A. Babul, P. F. Hopkins, R. Davé, B. Moa. 2019. Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem. MNRAS, 483, pp. 3810-3831. en_US
dc.description.scholarlevel Graduate en_US

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