Characterization of locally rotationally symmetric space-times

DOI10.1007/BF00765890zbMath0584.53029MaRDI QIDQ1069472

John Wainwright, Stephen W. Goode

Publication date: 1986

Published in: General Relativity and Gravitation (Search for Journal in Brave)

zbMATH Keywords

Einstein equationstetrad formalismlocally rotationally symmetric space-times

Mathematics Subject Classification ID

Applications of local differential geometry to the sciences (53B50) Local differential geometry of Lorentz metrics, indefinite metrics (53B30)

Related Items (10)

Shear-free perfect fluids in general relativity. I. Petrov type N Weyl tensor ⋮ Cosmological models ⋮ Observer-based invariants for cosmological models ⋮ Inhomogeneous spacetimes in Einstein-æther cosmology ⋮ Quantization of inhomogeneous spacetimes with cosmological constant term ⋮ Poynting vector, super-Poynting vector, and principal observers in electromagnetism and general relativity ⋮ Spacetimes with continuous linear isotropies. I: Spatial rotations ⋮ Spacetimes with continuous linear isotropies. II: Boosts ⋮ Quantum cosmology of a Bianchi III LRS geometry coupled to a source free electromagnetic field ⋮ The Maple package NPTOOLS; a symbolic algebra package for tetrad formalisms in general relativity

Cites Work

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• Classification of the type D perfect-fluid solutions of the Einstein equations
• A review of the geometrical equivalence of metrics in general relativity
• A class of inhomogeneous cosmological models
• A class of homogeneous cosmological models
• Lorentzian 4 dimensional manifolds with 'local isotropy'
• A class of shear-free perfect fluids in general relativity. II
• An Approach to Gravitational Radiation by a Method of Spin Coefficients
• Space-times homogeneous on a time-like hypersurface
• Inhomogeneous cosmologies: New exact solutions and their evolution

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