Black-Hole Lattices as Cosmological Models
arXiv:1801.01083 · doi:10.1088/1361-6382/aac846
Abstract
The search for solutions of Einstein's equations representing relativistic cosmological models with a discrete matter content has been remarkably fruitful in the last decade. In this review we discuss the progress made in the study of a specific subclass of discrete cosmologies, Black-Hole Lattice models. In particular, we illustrate the techniques used for the construction of these spacetimes, and examine their resulting physical properties. This includes their large-scale dynamics, the dressing of mass due to the interaction between individual black holes, along with features of direct observational interest such as the distance-to-redshift relation. This collection of results provides a novel perspective on the physical effects of averaging in General Relativity, as well as on the emergence of gravitational structures from solutions with isolated objects.
54 pages, 16 figures, review prepared for the CQG Special Focus Issue "Computational issues in mathematical cosmology"
References in corpus (11)
- Binary black hole merger dynamics and waveforms
- Foundations of multiple black hole evolutions
- Inhomogeneous Cosmology with Numerical Relativity
- Close encounters of three black holes
- Numerical evolution of multiple black holes with accurate initial data
- Construction of N-body initial data sets in general relativity
- The Averaging Problem in Cosmology and Macroscopic Gravity
- Choreographic solution to the general relativistic three-body problem
- The Magnetic Part of the Weyl Tensor, and the Expansion of Discrete Universes
- Exact Initial Data for Black Hole Universes with a Cosmological Constant
- Cosmological Solutions with Charged Black Holes
Cited by in corpus (19)
- The Limited Accuracy of Linearized Gravity
- CTTK: A new method to solve the initial data constraints in numerical relativity
- General Relativistic Cosmological N-body Simulations I: time integration
- Gravitational Collapse of a Massless Scalar Field in a Periodic Box
- Cosmology using numerical relativity
- Gauss-Bonnet-Chern approach to the averaged Universe
- The effect of dark matter discreteness on light propagation
- Cosmic expansion from spinning black holes
- Perturbatively constructed cosmological model with periodically distributed dust inhomogeneities
- Einstein clusters as models of inhomogeneous spacetimes
- Structure formation and quasi-spherical collapse from initial curvature perturbations with numerical relativity simulations
- Sound waves from primordial black hole formations
- On the intrinsically flat cosmological models in a lattice
- Intrinsically symmetric cosmological model in the presence of dissipative fluids
- Lie sphere-geometry in lattice cosmology
- Construction of the cosmological model with periodically distributed inhomogeneities with growing amplitude
- Discrete Cosmological Models in the Brans-Dicke Theory of Gravity
- Analytic Analysis of Irregular Discrete Universes
- A Gravitational Wave Background from Primordial Black Hole Lattices in Matter Dominated Era