CMB in the river frame and gauge invariance at second order
arXiv:1708.00441 · doi:10.1088/1475-7516/2018/03/014
Abstract
GAUGE INVARIANCE: The Sachs-Wolfe formula describing the Cosmic Microwave Background (CMB) temperature anisotropies is one of the most important relations in cosmology. Despite its importance, the gauge invariance of this formula has only been discussed at first order. Here we discuss the subtle issue of second-order gauge transformations on the CMB. By introducing two rules (needed to handle the subtle issues), we prove the gauge invariance of the second-order Sachs-Wolfe formula and provide several compact expressions which can be useful for the study of gauge transformations on cosmology. Our results go beyond a simple technicality: we discuss from a physical point of view several aspects that improve our understanding of the CMB. We also elucidate how crucial it is to understand gauge transformations on the CMB in order to avoid errors and/or misconceptions as occurred in the past. THE RIVER FRAME: we introduce a cosmological frame which we call the river frame. In this frame, photons and any object can be thought as fishes swimming in the river and relations are easily expressed in either the metric or the covariant formalism then ensuring a transparent geometric meaning. Finally, our results show that the river frame is useful to make perturbative and non-perturbative analysis. In particular, it was already used to obtain the fully nonlinear generalization of the Sachs-Wolfe formula and is used here to describe second-order perturbations.
29 pages, 2 figures, references added, sec. 2.1 enhanced, appendix B added, published in JCAP
References in corpus (11)
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
- Sachs-Wolfe at second order: the CMB bispectrum on large angular scales
- Cosmological Perturbations at Second Order and Recombination Perturbed
- Action approach to cosmological perturbations: the 2nd order metric in matter dominance
- Gauging the cosmic microwave background
- General treatment of isocurvature perturbations and non-Gaussianities
- CMB Anisotropies from a Gradient Mode
- Interpreting the CMB aberration and Doppler measurements: boost or intrinsic dipole?
- CMB anisotropies at all orders: the non-linear Sachs-Wolfe formula
- Statistics of the CMB polarised anisotropies