Cosmic expansion from spinning black holes

DOI10.1088/1361-6382/ab3bf2zbMath1478.83153arXiv1903.01490OpenAlexW3106420743MaRDI QIDQ5159957

John T. Giblin Jr, Glenn D. Starkman, Chi Tian, James B. Mertens

Publication date: 28 October 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1903.01490

zbMATH Keywords

inhomogeneous cosmologyKerr black holenumerical relativityFLRW universeblack hole lattice

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Lattice gravity, Regge calculus and other discrete methods in general relativity and gravitational theory (83C27) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Motion of the gyroscope (70E05)

Related Items (5)

CTTK: a new method to solve the initial data constraints in numerical relativity ⋮ Evolution of black holes through a nonsingular cosmological bounce ⋮ General relativistic cosmological N-body simulations. Part I. Time integration ⋮ Oscillon preheating in full general relativity ⋮ Relativistic quantum motion of an electron in spinning cosmic string spacetime in the presence of uniform magnetic field and Aharonov-Bohm potential

Uses Software

• AHFinderDirect

Cites Work

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