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Gravitational waves in general relativity: XIV. Bondi expansions and the ``polyhomogeneity'' of \Scri

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TLDR
In this paper, the structure of polyhomogeneous space-times with metrics which admit an expansion in terms of $r^{-j}\log^i r$ is analyzed, and the occurrence of some log terms in an asymptotic expansion of the metric is related to the non vanishing of the Weyl tensor at Scri.
Abstract
The structure of polyhomogeneous space-times (i.e., space-times with metrics which admit an expansion in terms of $r^{-j}\log^i r$) constructed by a Bondi--Sachs type method is analysed. The occurrence of some log terms in an asymptotic expansion of the metric is related to the non--vanishing of the Weyl tensor at Scri. Various quantities of interest, including the Bondi mass loss formula, the peeling--off of the Riemann tensor and the Newman--Penrose constants of motion are re-examined in this context.

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Isolated and dynamical horizons and their applications

TL;DR: A new, quasi-local framework was introduced to analyze diverse facets of black holes in a unified manner that has introduced a more physical setting for black hole thermodynamics, suggested a phenomenological model for hairy black holes, provided novel techniques to extract physics from numerical simulations, and led to new laws governing the dynamics ofblack holes in exact general relativity.
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Aspects of the BMS/CFT correspondence

TL;DR: In this paper, the symmetry algebra of asymptotically flat spacetimes at null infinity in 4 dimensions is taken to be the semi-direct sum of supertranslations with infinitesimal local conformal transformations.
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Isolated horizons: Hamiltonian evolution and the first law

TL;DR: In this article, a framework was introduced to generalize black hole mechanics by replacing stationary event horizons with isolated horizons and the boundary conditions now allow the horizon to be distorted and rotating, and subsequent analysis is based on several new ingredients.
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Black hole boundaries

TL;DR: In this paper, quasilocal characterizations of black holes are proposed for the causal past of future null infinity, where the event horizon is defined as a nonlocal object.
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A 3+1 perspective on null hypersurfaces and isolated horizons

TL;DR: In this article, a hierarchy of geometrical structures is constructed on a null hypersurface, and the isolated horizon structure is reformulated in this framework by making use of some 3 + 1 slicing of spacetime.
References
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Book ChapterDOI

Asymptotic Structure of Space-Time

TL;DR: In this article, the authors define a solution as representing an isolated system if i) the mass density vanishes outside some compact set in the Euclidean 3-space, and ii) the Newtonian gravitational potential approaches zero in the limit far from that compact set.
Journal ArticleDOI

Some spherical gravitational waves in general relativity

TL;DR: In this paper, the class of metrics which admit a family of hypersurface-orthogonal, non-shearing, diverging null curves is studied. But their solutions admit no Killing field whatsoever.
Journal ArticleDOI

Reduction of the characteristic initial value problem to the Cauchy problem and its applications to the Einstein equations

TL;DR: In this article, it is shown that the characteristic initial value problem for the Einstein equations in vacuum or with perfect fluid source is well posed when data are given on two transversely intersecting null hypersurfaces.
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On the regularity of solutions to the Yamabe equation and the existence of smooth hyperboloidal initial data for Einstein's field equations

TL;DR: The regularity of the solutions to the Yamabe Problem in the case of conformally compact manifolds and negative scalar curvature is investigated in this article, and the existence of smooth hyperboloidal initial data for Einstein's field equations is demonstrated.
Journal ArticleDOI

The problem of a self-gravitating scalar field

TL;DR: In this article, the authors studied the global initial value problem for the spherically symmetric case with a massless scalar field as the material model and proved the local, in retarded time, existence and global uniqueness of classical solutions.
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