Spinning boson stars and Kerr black holes with scalar hair: the effect of self-interactions
Self-interacting boson stars (BSs) have been shown to alleviate the astrophysically low maximal mass of their nonself-interacting counterparts. We report some physical features of spinning self-interacting BSs, namely their compactness, the occurrence of ergo-regions and the scalar field profiles, f...
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| Outros Autores: | , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2016
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| Assuntos: | |
| Texto completo: | http://hdl.handle.net/10773/16898 |
| País: | Portugal |
| Oai: | oai:ria.ua.pt:10773/16898 |