A fully covariant description of cosmic microwave background anisotropies

DOI10.1088/0264-9381/14/12/021zbMath0904.53069arXivgr-qc/9707022OpenAlexW3121827652MaRDI QIDQ3839473

Peter K. S. Dunsby

Publication date: 9 August 1998

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9707022

zbMATH Keywords

Weyl tensorcosmic microwave background radiationtemperature anisotropymatter and radiation

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35)

Related Items (6)

The gravitational light shift and the Sachs-Wolfe effect ⋮ \(1+3\) covariant cosmic microwave background anisotropies. I: Algebraic relations for mode and multipole expansions ⋮ \(1+3\) covariant cosmic microwave background anisotropies. II: The almost Friedmann-Lemaître model ⋮ Workshop 2: Cosmic microwave background, lensing and large-scale structure ⋮ The covariant perturbative approach to cosmic microwave background anisotropies ⋮ CMB in the river frame and gauge invariance at second order

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