G1 Cosmologies with Gravitational and Scalar Waves
arXiv:gr-qc/9812069 · doi:10.1103/PhysRevD.60.104008
Abstract
I present here a new algorithm to generate families of inhomogeneous massless scalar field cosmologies. New spacetimes, having a single isometry, are generated by breaking the homogeneity of massless scalar field models along one direction. As an illustration of the technique I construct cosmological models which in their late time limit represent perturbations in the form of gravitational and scalar waves propagating on a non-static inhomogeneous background. Several features of the obtained metrics are discussed, such as their early and late time limits, structure of singularities and physical interpretation.
24 pages, 2 figures
References in corpus (8)
- Self-Similarity in General Relativity \endtitle
- Mixmaster Behavior in Inhomogeneous Cosmological Spacetimes
- Evidence for an oscillatory singularity in generic U(1) symmetric cosmologies on
- The Singularity in Generic Gravitational Collapse Is Spacelike, Local, and Oscillatory
- Phenomenology of the Gowdy Universe on
- Numerical Evidence that the Singularity in Polarized U(1) Symmetric Cosmologies on is Velocity Dominated
- The Gowdy T3 Cosmologies revisited
- Inhomogeneous Einstein-Rosen String Cosmology
Cited by in corpus (7)
- Cosmology with exponential potentials
- Separable Brane Cosmologies in Heterotic M-Theory
- Inhomogeneous Einstein-Rosen String Cosmology
- Exact inhomogeneous Einstein-Maxwell-Dilaton cosmologies
- Solution generating in scalar-tensor theories with a massless scalar field and stiff perfect fluid as a source
- Dilatonic Domain Walls and Curved Intersecting Branes
- Asymptotic singular behaviour of inhomogeneous cosmologies in Einstein-Maxwell-dilaton-axion theory