Iron K alpha line of Proca stars
X-ray reflection spectroscopy can be a powerful tool to test the nature of astrophysical black holes. Extending previous work on Kerr black holes with scalar hair [1] and on boson stars [2], here we study whether astrophysical black hole candidates may be horizonless, self-gravitating, vector Bose-E...
| Autor principal: | |
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| Outros Autores: | , , , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
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| Assuntos: | |
| Texto completo: | http://hdl.handle.net/10773/21300 |
| País: | Portugal |
| Oai: | oai:ria.ua.pt:10773/21300 |