Explorations of the infinite regions of space-time
arXiv:2005.11936 · doi:10.1142/S0218271820300074
Abstract
An important concept in Physics is the notion of an isolated system. It is used in many different areas to describe the properties of a physical system which has been isolated from its environment. The interaction with the `outside' is then usually reduced to a scattering process, in which incoming radiation interacts with the system, which in turn emits outgoing radiation. In Einstein's theory of gravitation isolated systems are modeled as asymptotically flat space-times. They provide the appropriate paradigm for the study of gravitational waves and their interaction with a material system or even only with themselves. In view of the emerging era of gravitational wave astronomy, in which gravitational wave signals from many different astrophysical sources are detected and interpreted, it is necessary to have a foundation for the theoretical and numerical treatments of these signals. Furthermore, from a purely mathematical point of view, it is important to have a full understanding of the implications of imposing the condition of asymptotic flatness onto solutions of the Einstein equations. While it is known that there exists a large class of asymptotically flat solutions of Einstein's equations, it is not known what the necessary and sufficient conditions at infinity are that have to be imposed on initial data so that they evolve into regular asymptotically flat space-times. The crux lies in the region near space-like infinity where incoming and outgoing radiation `meet'. In this paper we review the current knowledge and some of the analytical and numerical work that has gone into the attempt to understand the structure of asymptotically flat space-times near space-like and null-infinity.
arXiv commentfinal version, consistent with published article
References in corpus (30)
- The linear stability of the Schwarzschild solution to gravitational perturbations
- Existence of non-trivial, vacuum, asymptotically simple space-times
- Spin-2 fields on Minkowski space near space-like and null infinity
- Asymptotically Flat Initial Data with Prescribed Regularity at Infinity
- On ``hyperboloidal'' Cauchy data for vacuum Einstein equations and obstructions to smoothness of ``null infinity''
- Future stability of the FLRW fluid solutions in the presence of a positive cosmological constant
- Conformal geodesics on vacuum space-times
- Peeling or not peeling -- is that the question ?
- Axisymmetric fully spectral code for hyperbolic equations
- Stabilizing relativistic fluids on spacetimes with non-accelerated expansion
- Constraints as evolutionary systems
- A Fully Pseudospectral Scheme for Solving Singular Hyperbolic Equations
- Global simulations of Minkowski space-time including space-like infinity
- The second order spin-2 system in flat space near space-like and null-infinity
- Numerical space-times near space-like and null infinity. The spin-2 system on Minkowski space
- Asymptotic simplicity and static data
- Fully pseudospectral time evolution and its application to 1+1 dimensional physical problems
- A rigidity property of asymptotically simple spacetimes arising from conformally flat data
- Perturbative Solutions of the Extended Constraint Equations in General Relativity
- Fully pseudospectral solution of the conformally invariant wave equation near the cylinder at spacelike infinity
- Fully pseudospectral solution of the conformally invariant wave equation near the cylinder at spacelike infinity. II: Schwarzschild background
- Conformal structures of static vacuum data
- The interior of axisymmetric and stationary black holes: Numerical and analytical studies
- Asymptotics of solutions of a hyperbolic formulation of the constraint equations
- Numerical construction of initial data sets of binary black hole type using a parabolic-hyperbolic formulation of the vacuum constraint equations
- Spectral methods for the spin-2 equation near the cylinder at spatial infinity
- Fully pseudospectral solution of the conformally invariant wave equation near the cylinder at spacelike infinity. III: Nonspherical Schwarzschild waves and singularities at null infinity
- On solving the constraints by integrating a strongly hyperbolic system
- Numerical initial data deformation exploiting a gluing construction: I. Exterior asymptotic Schwarzschild
- Linear Wave Equations on Lorentzian Manifolds