Evolution of black holes through a nonsingular cosmological bounce

DOI10.1088/1475-7516/2022/09/063OpenAlexW4297143106MaRDI QIDQ5041321

Justin Ripley, William E. East, Maxence Corman

Publication date: 13 October 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2206.08466

zbMATH Keywords

physics of the early universealternatives to inflationGR black holes

Mathematics Subject Classification ID

Black holes (83C57) Geometrodynamics and the holographic principle (83E05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) General theory of infinite-dimensional dissipative dynamical systems, nonlinear semigroups, evolution equations (37L05)

Uses Software

• AHFinderDirect

Cites Work

• Unnamed Item
• Unnamed Item
• Null energy condition and superluminal propagation
• Adaptive mesh refinement for hyperbolic partial differential equations
• Supersmoothing through slow contraction
• Adaptive mesh refinement for coupled elliptic-hyperbolic systems
• Event and apparent horizon finders for \(3+1\) numerical relativity
• Holography in general space-times
• Gravitational collapse: The role of general relativity
• Isolated and dynamical horizons and their applications
• Nonlinear dynamics of flux compactification
• Conformal structure of a Schwarzschild black hole immersed in a Friedman universe
• Cosmological and black hole apparent horizons
• Fully stable cosmological solutions with a non-singular classical bounce
• Bouncing cosmologies: progress and problems
• A critical review of classical bouncing cosmologies
• The four laws of black hole mechanics
• Some uniqueness results for dynamical horizons
• The cosmological higgstory of the vacuum instability
• Dynamical Horizons: Energy, Angular Momentum, Fluxes, and Balance Laws
• Evolution of a periodic eight-black-hole lattice in numerical relativity
• Marginally trapped tubes and dynamical horizons
• EXISTENCE OF BLACK HOLES IN FRIEDMANN–ROBERTSON–WALKER UNIVERSE DOMINATED BY DARK ENERGY
• Black Hole Singularities: A Numerical Approach
• Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
• A point mass in an isotropic universe: Existence, uniqueness, and basic properties
• Cosmological perturbations in a big-crunch–big-bang space-time
• Numerical relativity using a generalized harmonic decomposition
• A point mass in an isotropic universe: II. Global properties
• The Mass-Particle in an Expanding Universe
• PERSISTENCE OF BLACK HOLES THROUGH A COSMOLOGICAL BOUNCE
• A point mass in an isotropic universe: III. The region Rleq 2 m
• Robustness of inflation to inhomogeneous initial conditions
• Unbraiding the bounce: superluminality around the corner
• The effects of potential shape on inhomogeneous inflation
• Robustness of slow contraction to cosmic initial conditions
• Cosmic expansion from spinning black holes
• Traversable $ \newcommand{\e}{{\rm e}} \ell$ -wormholes supported by ghost scalar fields
• Persistent black holes in bouncing cosmologies
• Simulation of binary black hole spacetimes with a harmonic evolution scheme
• The Large Scale Structure of Space-Time
• Minimal conditions for the creation of a Friedman-Robertson-Walker universe from a bounce

This page was built for publication: Evolution of black holes through a nonsingular cosmological bounce