Republication of: Perturbations of a cosmological model and angular variations of the microwave background. Edited and with commentary by George Ellis and with notes on Sachs-Wolfe integration by Jürgen Ehlers. With brief autobiographies by Sachs and Wol

DOI10.1007/s10714-007-0448-9zbMath1150.83002OpenAlexW2012481663MaRDI QIDQ2461566

A. M. Wolfe

Publication date: 28 November 2007

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

Full work available at URL: https://doi.org/10.1007/s10714-007-0448-9

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) History of relativity and gravitational theory (83-03) Astrophysical cosmology (85A40)

Related Items (19)

Effective field theory of dark energy: a review ⋮ Relativistic angular redshift fluctuations embedded in large scale varying gravitational potentials ⋮ Second-order gauge-invariant formalism for the cosmological observables: complete verification of their gauge-invariance ⋮ Primordial clocks within stochastic gravitational wave anisotropies ⋮ Bumblebee field as a source of cosmological anisotropies ⋮ Covariant decomposition of the non-linear galaxy number counts and their monopole ⋮ Deformation of the gravitational wave spectrum by density perturbations ⋮ The art of building a smooth cosmic distance ladder in a perturbed universe ⋮ Non-Gaussianity in the squeezed three-point correlation from the relativistic effects ⋮ Momentum transfer models of interacting dark energy ⋮ Probing modified gravity with integrated Sachs-Wolfe CMB and galaxy cross-correlations ⋮ Primordial non-Gaussianity f_NLand anisotropies in scalar-induced gravitational waves ⋮ Brans–Dicke cosmology with a Λ-term: a possible solution to ΛCDM tensions* ⋮ GALILEAN COVARIANCE AND THE GRAVITATIONAL FIELD ⋮ On structure formation from a small-scales-interacting dark sector ⋮ CMB anisotropies at all orders: the non-linear Sachs-Wolfe formula ⋮ Probing the imprints of generalized interacting dark energy on the growth of perturbations ⋮ CMB in the river frame and gauge invariance at second order ⋮ Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen

Cites Work

• Microwave background anisotropies from gravitational waves: the 1 + 3 covariant approach
• C$^{\,\infty}$ perturbations of FRW models with a cosmological constant
• The cosmic microwave background
• Computational cosmology: from the early universe to the large scale structure

This page was built for publication: Republication of: Perturbations of a cosmological model and angular variations of the microwave background. Edited and with commentary by George Ellis and with notes on Sachs-Wolfe integration by Jürgen Ehlers. With brief autobiographies by Sachs and Wol