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...

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Bibliographic Details
Main Author: Shen, T. L. (author)
Other Authors: Zhou, M. L. (author), Bambi, C. (author), Herdeiro, C. A. R. (author), Radu, E. (author)
Format: article
Language:eng
Published: 1000
Subjects:
Astrophysical black holes
Gravity
X-rays
Online Access:http://hdl.handle.net/10773/21300
Country:Portugal
Oai:oai:ria.ua.pt:10773/21300

Internet

http://hdl.handle.net/10773/21300

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