[PDF] Top 20 On the classification of stationary electro-vacuum black holes
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On the classification of stationary electro-vacuum black holes
... with the existing literature is in order; we focus on those points that do not generalize immediately when passing from pure to ...First of all, the famous reduction of the ... See full document
25
Spinning black holes in shift-symmetric Horndeski theory
... spinning black holes (BHs) in shift-symmetric Horndeski ...wherein the (real) scalar field couples lin- early to the Gauss-Bonnet curvature squared ...combination. The BH solutions ... See full document
32
Black holes in a box: Toward the numerical evolution of black holes in AdS space-times
... simulations of BH binaries by computing the Weyl scalar 4 , which has the asymptotic property of being equal to the outgoing radiation if the complex null tetrad is chosen ... See full document
17
Horizon geometry for Kerr black holes with synchronized hair
... study the horizon geometry of a generalization of the Kerr solution and, in particular, its embedding in E 3 .... The generalized Kerr BHs we shall be considering are Kerr BHs with ... See full document
9
Shadows of Einstein-dilaton-Gauss-Bonnet black holes
... how the dGB term impacts on one particular observable feature of a BH: its shadow [26] ...as the silhouette produced by the BH when placed in front of a bright ...by the ... See full document
7
Einstein-Maxwell-scalar black holes: The hot, the cold and the bald
... to the extremal RN BH. The second branch (hot scalarised BHs) connects to the first one at the minimum value of the charge to mass ratio and it includes overcharged ...assess ... See full document
8
Shadows of exact binary black holes
... in the double-Schwarzschild BH solutions. In the latter case, it was observed in [18] that thanks to the underlying cylindrical symmetry, of both the geometry and the spatial ... See full document
9
Inside black holes with synchronized hair
... for the stationary scalar clouds on Kerr, i.e. smoothness on the event horizon and strong oscilla- tions near the Cauchy horizon, should be generic for any test field obeying ... See full document
9
Spontaneous scalarization of charged Black Holes
... scalarization of vacuum black holes ...class of models, which includes, ...scalarization of electrovacuum BHs should ...compute the nonspherical sector of static ... See full document
6
Reissner-Nordstrom black holes with non-Abelian hair
... where the gauge sector is augmented by higher order terms. Linearising the (extended) Yang–Mills equations on the background of the electric Reissner–Nordström (RN) black ... See full document
7
Kerr–Newman black holes with scalar hair
... discovered, the Kerr solution admits also families of generalizations with scalar hair [12–16] (and also Proca hair [17] ...distribution of a com- plex, massive scalar field can be added to Kerr BHs, ... See full document
8
On the Field of a Stationary Charged Spherical Source
... equations of gravitation related to the field of a spherical charged source imply the existence of an interdependence between gravitation and electricity ...[5]. The present ... See full document
6
AdS Black Holes from Localized Boundary Sources
... [1], the authors solved the Einstein-Maxwell equations with a negative cos- mological constant for a stationary and axisymetric spacetime, imposing that at the conformal boundary the ... See full document
60
Elementary particles under the lens of the black holes
... considered the first piece of this series of theorems, namely, every rotation- less black hole should be spherically symmetric ...extend the analysis to ro- tating black ... See full document
5
Kerr black holes with scalar and Proca hair
... in the current literature of black holes statements that stationary black holes in General Relativity are described solely by mass, angular momentum and ...and the ... See full document
141
Stationary scalar clouds around a BTZ black hole
... establish the existence of stationary clouds of massive test scalar fields around BTZ black ...zero-modes of the superradiant instability and are possible when Robin ... See full document
6
On uniqueness of stationary vacuum black holes
... with the existing literature are in order. First, the event horizon in a smooth or analytic black hole space-time is a priori only a Lipschitz surface, which is way insufficient to prove the ... See full document
60
Astrophysical imaging of Kerr black holes with scalar hair
... address the astrophysical imaging of a family of deformed Kerr black holes ...are stationary, asymptotically flat BH spacetimes that are solutions of general relativity ... See full document
12
Spherical electro-vacuum black holes with resonant, scalar Q-hair
... It turns out, however, that there are no zero modes of the instability that are also bound states.5 This was shown by Hod in the case of a test, massive, charged scalar field on the RN b[r] ... See full document
13
Stationary Black Holes and Light Rings
... shadow of the astrophysically significant Kerr black hole (BH) are both intimately connected to a special set of bound null orbits known as light rings ...prove the following theorem. A ... See full document
5
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