Equivalence classes of perturbations in cosmologies of Bianchi types I and V: Interpretation

DOI10.1063/1.532958zbMath0952.83044OpenAlexW4251111795WikidataQ125305801 ScholiaQ125305801MaRDI QIDQ4270396

Zbigniew Banach

Publication date: 21 November 1999

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.532958

zbMATH Keywords

semiclassical descriptiongauge-invariant variableanisotropic background modelsequivalence classes of perturbations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

Equivalence classes of perturbations in cosmologies of Bianchi types I and V: Formulation

Cites Work

• Gauge-invariant cosmological perturbation theory for collisionless matter: Application to the Einstein-Liouville system
• Geometrization of linear perturbation theory for diffeomorphism-invariant covariant field equations. I: The notion of a gauge-invariant variable
• Geometrization of linear perturbation theory for diffeomorphism-invariant covariant field equations. II: Basic gauge-invariant variables with applications to de Sitter space-time
• General covariance in general relativity?
• Gauge-invariant perfect-fluid Robertson-Walker perturbations
• Perturbations of Friedmann-Robertson-Walker cosmological models
• Local symmetries and constraints
• Equivalence classes of perturbations in cosmologies of Bianchi types I and V: Formulation
• The symplectic geometry of a parametrized scalar field on a curved background
• Perennials and the group-theoretical quantization of a parametrized scalar field on a curved background

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