Numerical simulations of Gowdy spacetimes on S2×S1×R

David Garfinkle
Phys. Rev. D 60, 104010 – Published 15 October 1999
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Abstract

Numerical simulations are performed of the approach to the singularity in Gowdy spacetimes on S2×S1×R. The behavior is similar to that of Gowdy spacetimes on T3×R. In particular, the singularity is asymptotically velocity term dominated, except at isolated points where spiky features develop.

  • Received 7 June 1999

DOI:https://doi.org/10.1103/PhysRevD.60.104010

©1999 American Physical Society

Authors & Affiliations

David Garfinkle*

  • Department of Physics, Oakland University, Rochester, Michigan 48309

  • *Email address: garfinkl@oakland.edu

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Issue

Vol. 60, Iss. 10 — 15 November 1999

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