Numerical Evidence that the Singularity in Polarized U(1) Symmetric Cosmologies on $T^3 \times R$ is Velocity Dominated

Details Numerical Evidence that the Singularity in Polarized U(1) Symmetric Cosmologies on $T^3 \times R$ is Velocity Dominated Numerical Evidence that the Singularity in Polarized U(1) Symmetric Cosmologies on $T^3 \times R$ is Velocity Dominated

1998-01-22

arxiv.org/abs/gr-qc/9801078v1

Phys.Rev. D57 (1998) 7235-7240

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, RevTex, 4 figures, uses epsf

Scientific paper

10.1103/PhysRevD.57.7235

Numerical evidence supports the conjecture that polarized U(1) symmetric
cosmologies have asymptotically velocity term dominated singularities.

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