On the area of the symmetry orbits in T 2 symmetric spacetimes with Vlasov matter
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Publication:4466977
DOI10.1088/0264-9381/21/4/023zbMath1054.83007arXivgr-qc/0308055OpenAlexW1988000295MaRDI QIDQ4466977
Publication date: 8 June 2004
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0308055
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
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Areal foliation and asymptotically velocity-term dominated behavior in T2 symmetric space-times with positive cosmological constant ⋮ The Einstein-Vlasov-scalar field system with Gowdy or \(T^2\) symmetry in contracting direction ⋮ LOCAL EXISTENCE AND CONTINUATION CRITERIA FOR SOLUTIONS OF THE EINSTEIN–VLASOV-SCALAR FIELD SYSTEM WITH SURFACE SYMMETRY ⋮ A global foliation of Einstein-Euler spacetimes with Gowdy-symmetry on \(T ^{3}\) ⋮ The Einstein-Vlasov system/kinetic theory ⋮ Theorems on existence and global dynamics for the Einstein equations ⋮ Strong Cosmic Censorship for Surface-Symmetric Cosmological Spacetimes with Collisionless Matter ⋮ Static spherically symmetric Einstein-Vlasov bifurcations of the Schwarzschild spacetime
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