Phys. Rev. D 57, 7235–7240 (1998)

Numerical evidence that the singularity in polarized U(1) symmetric cosmologies on T³×R is velocity dominated

Abstract

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Beverly K. Berger^*
Department of Physics, Oakland University, Rochester, Michigan 48309

Vincent Moncrief^†
Departments of Physics and Mathematics, Yale University, New Haven, Connecticut 06520

Received 26 January 1998; published in the issue dated 15 June 1998

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

URL:

http://link.aps.org/doi/10.1103/PhysRevD.57.7235

DOI:

10.1103/PhysRevD.57.7235

PACS:

98.80.Hw, 04.20.Jb

^*Email address: berger@oakland.edu

^†Email address: moncrief@hepvms.physics.yale.edu

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Phys. Rev. D 57, 7235–7240 (1998)

Numerical evidence that the singularity in polarized U(1) symmetric cosmologies on T3×R is velocity dominated

Numerical evidence that the singularity in polarized U(1) symmetric cosmologies on T³×R is velocity dominated