Cosmology in three dimensions: steps towards the general solution

DOI10.1088/0264-9381/23/17/012zbMath1100.83034arXivgr-qc/0606025OpenAlexW1985540895MaRDI QIDQ5489748

Douglas J. Shaw, John D. Barrow, Christos G. Tsagas

Publication date: 28 September 2006

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0606025

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Analogues of general relativity in lower dimensions (83C80) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (12)

On scalar curvature invariants in three dimensional spacetimes ⋮ Dirac field as a source of the inflation in \(2 + 1\) dimensional teleparallel gravity ⋮ Two Fluids Cosmological Model in (2+1)-Dimensional Saez-Ballester Scalar-Tensor Theory of Gravitation ⋮ Solutions for the null-surface formulation in \(2+1\) dimensions leading to spacetimes of Petrov types i, II, and D ⋮ Three-variable solution in the \((2+1)\)-dimensional null-surface formulation ⋮ Topology and incompleteness for 2+1-dimensional cosmological spacetimes ⋮ A de Sitter no-hair theorem for 3+1d cosmologies with isometry group forming 2-dimensional orbits ⋮ Radiation in \((2 + 1)\)-dimensions ⋮ Some static spherically symmetric interior solutions of \(f (R)\) gravity ⋮ Gödel type metrics in three dimensions ⋮ All solutions of Einstein’s equations in 2+1 dimensions: Λ-vacuum, pure radiation, or gyratons ⋮ The generalized second law of thermodynamics for interacting f(R) gravity

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