Year: 2023
Type: dissertation
Abstract: Light scalar fields are the essence of many well-motivated theories beyond the Standard Model of particle physics. In this thesis, we study the rich phenomenology of the interplay between these fields and the finite baryon density present in astrophysical environments such as stars and supernovae. The emerging phenomena range from changes in QCD axion couplings to phase transitions from stars to changing the stellar landscape. Compatibility with observations allows us to put stringent constraints on such models.
Authors: Springmann, Konstantin F., Weiler, Andreas 1975-, Technische Universität München
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W7047819318
