A new inhomogeneous cosmological perfect fluid solution with p=ρ/3

DOI10.1088/0264-9381/6/6/001zbMath1248.83011OpenAlexW2016967805MaRDI QIDQ2918522

José M. M. Senovilla, Alexander Feinstein

Publication date: 6 October 2012

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

Full work available at URL: http://stacks.iop.org/0264-9381/6/L89

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (7)

Symmetry group analysis for perfect fluid inhomogeneous cosmological models in general relativity ⋮ Dynamical equilibrium states of a class of irrotational non-orthogonally transitive G ₂ cosmologies: II. Models with one hypersurface-orthogonal Killing vector field ⋮ Dynamical equilibrium states of a class of irrotational non-orthogonally transitive G ₂ cosmologies I: The conjecture of chaotic cosmological inhomogeneity ⋮ A big-bang cylindrically symmetric radiation universe ⋮ Singularity theorems and their consequences ⋮ New class of inhomogeneous cosmological perfect-fluid solutions without big-bang singularity ⋮ Nonsingular inhomogeneous string cosmology

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