Erratum: Slowly rotating black holes in dynamical Chern-Simons gravity: Deformation quadratic in the spin [Phys. Rev. D 86, 044037 (2012)]

2014 ◽  
Vol 89 (4) ◽  
Author(s):  
Kent Yagi ◽  
Nicolás Yunes ◽  
Takahiro Tanaka
2006 ◽  
Vol 21 (35) ◽  
pp. 2621-2635 ◽  
Author(s):  
JUTTA KUNZ ◽  
FRANCISCO NAVARRO-LÉRIDA

Stationary black holes in five-dimensional Einstein–Maxwell–Chern–Simons theory possess surprising properties. When considering the Chern–Simons coefficient λ as a parameter, two critical values of λ appear: the supergravity value λ SG = 1, and the value λ = 2. At λ = 1, supersymmetric black holes with vanishing horizon angular velocity, but finite angular momentum exist. As λ increases beyond λ SG a rotational instability arises, and counterrotating black holes appear, whose horizon rotates in the opposite sense to the angular momentum. Thus supersymmetry is associated with the borderline between stability and instability. At λ = 2, rotating black holes with vanishing angular momentum emerge. Beyond λ = 2, black holes may possess a negative horizon mass, while their total mass is positive. Charged rotating black holes with vanishing gyromagnetic ratio appear, and black holes are no longer uniquely characterized by their global charges.


2021 ◽  
Vol 104 (6) ◽  
Author(s):  
Stephon Alexander ◽  
Gregory Gabadadze ◽  
Leah Jenks ◽  
Nicolás Yunes

2015 ◽  
Vol 92 (4) ◽  
Author(s):  
Jose Luis Blázquez-Salcedo ◽  
Jutta Kunz ◽  
Francisco Navarro-Lérida ◽  
Eugen Radu

2013 ◽  
Vol 87 (2) ◽  
Author(s):  
L. Bonora ◽  
M. Cvitan ◽  
P. Dominis Prester ◽  
S. Pallua ◽  
I. Smolić

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