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by Huangyu Xiao
| Institution: | University of Washington |
|---|---|
| Department: | |
| Degree: | PhD |
| Year: | 2022 |
| Keywords: | Axinovae; Axion minicluster; Axion stars; Particle physics; Astrophysics; Theoretical physics; Physics |
| Posted: | 3/25/2025 |
| Record ID: | 2298263 |
| Full text PDF: | http://hdl.handle.net/1773/49429 |
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.
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