The Axion Universe
| dc.contributor.advisor | Sharpe, Stephen | |
| dc.contributor.author | Xiao, Huangyu | |
| dc.date.accessioned | 2022-09-23T20:48:23Z | |
| dc.date.available | 2022-09-23T20:48:23Z | |
| dc.date.issued | 2022-09-23 | |
| dc.date.submitted | 2022 | |
| dc.description | Thesis (Ph.D.)--University of Washington, 2022 | |
| dc.description.abstract | The standard models of cosmology and particle physics have met enormous success. However,there are still a few big questions that remain to be answered. One of these outstanding questions is “what is the dark matter?”. One of the most well-motivated dark matter candidates is the axion, as it provides a natural solution to another fundamental problem called the strong CP problem. Axions can also be motivated by various theories in high energy physics. A Universe with axion dark matter is very colorful as one expects many planetary-mass collapsed structures and potentially compact clumps such as axion stars. Astrophysical and cosmological observations can be sensitive to these structures, providing a unique window into the nature of dark matter. We will discuss recent progress in the evolution, formation, and detectable signals of axion minihalos and axion stars. | |
| dc.embargo.terms | Open Access | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.other | Xiao_washington_0250E_24700.pdf | |
| dc.identifier.uri | http://hdl.handle.net/1773/49429 | |
| dc.language.iso | en_US | |
| dc.rights | none | |
| dc.subject | Axinovae | |
| dc.subject | Axion minicluster | |
| dc.subject | Axion stars | |
| dc.subject | Particle physics | |
| dc.subject | Astrophysics | |
| dc.subject | Theoretical physics | |
| dc.subject.other | Physics | |
| dc.title | The Axion Universe | |
| dc.type | Thesis |
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