Gowdy phenomenology in scale-invariant variables
arXiv:gr-qc/0310127 · doi:10.1088/0264-9381/21/3/003
Abstract
The dynamics of Gowdy vacuum spacetimes is considered in terms of Hubble-normalized scale-invariant variables, using the timelike area temporal gauge. The resulting state space formulation provides for a simple mechanism for the formation of ``false'' and ``true spikes'' in the approach to the singularity, and a geometrical formulation for the local attractor.
33 pages, 17 figures. To appear in A Spacetime Safari: Papers in Honour of Vincent Moncrief
References in corpus (16)
- Numerical Investigation of Cosmological Singularities
- E_(10), BE_(10) and Arithmetical Chaos in Superstring Cosmology
- The Bianchi IX attractor
- General Relativistic 1+3 Orthonormal Frame Approach Revisited
- Analytic description of singularities in Gowdy spacetimes
- The past attractor in inhomogeneous cosmology
- Asymptotic Behavior of the Gowdy Spacetimes
- The Singularity in Generic Gravitational Collapse Is Spacelike, Local, and Oscillatory
- Phenomenology of the Gowdy Universe on
- Manufacture of Gowdy spacetimes with spikes
- Oscillatory approach to the singularity in vacuum spacetimes with isometry
- Asymptotic expansions close to the singularity in Gowdy spacetimes
- Dynamical systems approach to G2 cosmology
- Asymptotic dynamics of the exceptional Bianchi cosmologies
- High velocity spikes in Gowdy spacetimes
- Approach to the Singularity in Spatially Inhomogeneous Cosmologies
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- Second-order hyperbolic Fuchsian systems. Asymptotic behavior of geodesics in Gowdy spacetimes
- Asymptotics and singularities in cosmological models with positive cosmological constant
- Quantum Cosmological Metroland Model
- Cylindrical gravitational waves in expanding universes: Models for waves from compact sources