[PDF] Top 20 Shadows of exact binary black holes
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Shadows of exact binary black holes
... their shadows, of general-relativistic BBHs is, however, more challenging than for isolated ...top of dynamical fully nonlinear numerical simulations. Specific features of the shadows ... See full document
9
Fundamental photon orbits: Black hole shadows and spacetime instabilities
... standard black holes (BHs) in general relativity, as well as other ultracompact objects (with or without an event horizon) admit planar circular photon ...regardless of the integrability properties ... See full document
6
Black holes in a box: Toward the numerical evolution of black holes in AdS space-times
... amount of gravitational wave energy radiated during the last stages of the inspiral, plunge, and merger of a corresponding binary system in an asymptotically flat space-time which is about ... See full document
17
Born-infeld corrections to the entropy function of heterotic black holes
... part of the Born- Infeld terms to the ...get exact analytical results when other types of gauge-gravitational terms are included in the ...an exact calculation to all orders in α ′ for the ... See full document
9
Elementary particles under the lens of the black holes
... beginning of the black hole golden era. From the theoretical point of view, ...that black holes must have a singularity in their interior ...exist binary systems formed by an ... See full document
5
Iron K alpha line of Kerr black holes with Proca hair
... spectra of Configuration IV and Configuration V cannot be fitted with a Kerr ...minimum of the reduced χ 2 is a large number and there are no ...case of Configuration III, the fit is good and the ... See full document
11
Astrophysical imaging of Kerr black holes with scalar hair
... imaging of a family of deformed Kerr black holes ...solutions of general relativity minimally coupled to a massive, complex scalar field: Kerr BHs with scalar hair ...distinct ... See full document
12
Inside black holes with synchronized hair
... Kerr black hole (BH) [1] is the widely accepted theoretical model for describing astrophysical BH candidates [2] ...plunge of two BHs into a final Kerr BH, the ringdown of the lat- ter [4] being ... See full document
9
Kerr–Newman black holes with scalar hair
... 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, keeping them asymptotically flat and regular on ... See full document
8
Spontaneous scalarization of charged Black Holes
... understanding of these evolutions requires nonlinear numerical simulations; these are challenging, particularly if no symmetries are imposed, in view of the higher-curvature terms in ESTGB ...scalarization ... See full document
6
Shadows of Kerr Black Holes with Scalar Hair
... lensing of this hair resembles closely that of the ultracompact BS on the bottom left panel of ...disconnected shadows of the (single) BH occur: the largest ones (besides the main ... See full document
5
Shadows of Einstein-dilaton-Gauss-Bonnet black holes
... inconsistencies of Einstein’s General Rel- ativity, such as its non-renormalizability [1–3] and the existence of singularities, have since long motivated the suggestion that higher curvature corrections ... See full document
7
Rotating black holes in Eddington-inspired Born-Infeld gravity: an exact solution
... an exact, rotating charged black hole solution within Eddington-inspired Born-Infeld ...out of contractions of the metric with the Ricci tensor, and formulated in metric-affine spaces ... See full document
32
Synchronous frequencies of extremal Kerr black holes: Resonances, scattering, and stability
... QNMs of an extremal Kerr black hole was performed using a modification of the continued fraction method [76] ...frequency of the modes is exactly equal to the synchronous frequency, and ... See full document
10
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality
... theory of Kaluza [ 11 ] and Klein [ 12 ], soon after Einstein constructed General Relativity (GR) [ 13 ...scription of higher dimensional GR-inspired theories [ 14 ], as well as in supergravity, see ... See full document
27
Bopp–Podolsky black holes and the no-hair theorem
... generalization of Podolsky electrodynamics to curved space-times gives rise to two possible types of ...contraction of the Riemann tensor and the field ...replacement of Maxwell theory by ... See full document
9
Horizon geometry for Kerr black holes with synchronized hair
... Domain of existence of KBHsSH solutions with m ¼ 1 (dark blue and upper light blue shaded regions) in an M versus ΩH diagram, both in units of the scalar field mass ...lines of constant ΩH ... See full document
9
Reissner-Nordstrom black holes with non-Abelian hair
... realisation of these clouds corresponds to coloured, electrically charged BH solutions in EeYM theory, which are thermodynamically favoured over the RN ...instability of RN BHs that parallels the familiar ... See full document
7
Spinning black holes in shift-symmetric Horndeski theory
... spinning black holes (BHs) in shift-symmetric Horndeski ...overview of the parameter space of the solutions together with a study of their basic geometric and phenomenological ...BH ... See full document
32
Kerr black holes with scalar and Proca hair
... literature of black holes statements that stationary black holes in General Relativity are described solely by mass, angular momentum and ... at, black hole ...process of ... See full document
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