scholarly journals Motion of particles on a four-dimensional asymptotically AdS black hole with scalar hair

2015 ◽  
Vol 75 (10) ◽  
Author(s):  
P. A. González ◽  
Marco Olivares ◽  
Yerko Vásquez
Keyword(s):  
2014 ◽  
Vol 89 (8) ◽  
Author(s):  
Sourav Bhattacharya ◽  
Hideki Maeda
Keyword(s):  

2006 ◽  
Vol 74 (6) ◽  
Author(s):  
Cristián Martínez ◽  
Ricardo Troncoso

2016 ◽  
Vol 2016 (10) ◽  
pp. 024-024 ◽  
Author(s):  
Anne-Christine Davis ◽  
Ruth Gregory ◽  
Rahul Jha

2020 ◽  
Vol 101 (8) ◽  
Author(s):  
Bartlomiej Kiczek ◽  
Marek Rogatko
Keyword(s):  

2019 ◽  
Author(s):  
Athanasios Bakopoulos ◽  
George Antoniou ◽  
Panagiota Kanti

2003 ◽  
Vol 67 (2) ◽  
Author(s):  
Daniel Sudarsky ◽  
José Antonio González
Keyword(s):  

2016 ◽  
Vol 94 (4) ◽  
Author(s):  
Nicolas Sanchis-Gual ◽  
Juan Carlos Degollado ◽  
Carlos Herdeiro ◽  
José A. Font ◽  
Pedro J. Montero
Keyword(s):  

2014 ◽  
Vol 23 (12) ◽  
pp. 1442014 ◽  
Author(s):  
Carlos A. R. Herdeiro ◽  
Eugen Radu

We show that scalar hair can be added to rotating, vacuum black holes (BHs) of general relativity. These hairy black holes (HBHs) clarify a lingering question concerning gravitational solitons: Whether a BH can be added at the centre of a boson star (BS), as it typically can for other solitons. We argue that it can, but only if it is spinning. The existence of such HBHs is related to the Kerr superradiant instability triggered by a massive scalar field. This connection leads to the following conjecture: a (hairless) BH, which is afflicted by the superradiant instability of a given field, must allow hairy generalizations with that field.


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