Gauge-invariant perfect-fluid Robertson-Walker perturbations
From MaRDI portal
Publication:1915379
DOI10.1007/BF02082830zbMath0853.58105OpenAlexW2058023450MaRDI QIDQ1915379
Zbigniew Banach, Slawomir Piekarski
Publication date: 5 January 1997
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf02082830
Related Items (5)
Equivalence classes of perturbations in cosmologies of Bianchi types I and V: Formulation ⋮ Equivalence classes of perturbations in cosmologies of Bianchi types I and V: Interpretation ⋮ Theory of cosmological perturbations formulated in terms of a complete set of basic gauge-invariant quantities ⋮ Geometrization of linear perturbation theory for diffeomorphism-invariant covariant field equations. I: The notion of a gauge-invariant variable ⋮ Gauge-invariant cosmological perturbation theory for collisionless matter: Application to the Einstein-Liouville system
Cites Work
- Unnamed Item
- An exact anisotropic solution of the Einstein-Liouville equations
- On the existence of perturbed Robertson-Walker universes
- Relaxation-time approximation for a Boltzmann gas in Robertson-Walker universe models
- Two linearization procedures for the Boltzmann equation in a \(k=0\) Robertson-Walker space-time
- Theory of cosmological perturbations formulated in terms of a complete set of basic gauge-invariant quantities
- Instability of closed spaces in general relativity
- Complete sets of functions for perturbations of Robertson Walker cosmologies
- Perturbation theory based on the Einstein–Boltzmann system. I. Illustration of the theory for a Robertson–Walker geometry
- Perturbation theory based on the Einstein–Boltzmann system. II. Illustration of the theory for an almost-Robertson–Walker geometry
- The Large Scale Structure of Space-Time
- General Relativity
This page was built for publication: Gauge-invariant perfect-fluid Robertson-Walker perturbations
