The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
Open accessAbstract
We consider in detail the problem of gauge dependence that exists in relativistic perturbation theory, going beyond the linear approximation and treating second- and higher-order perturbations. We first derive some mathematical results concerning the Taylor expansion of tensor fields under the action of one-parameter families (not necessarily groups) of diffeomorphisms. Secondly, we define gauge invariance to an arbitrary order n. Finally, we give a generating formula for the gauge transformation to an arbitrary order and explicit rules to second and third order. This formalism can be used in any field of applied general relativity, such as cosmological and black hole perturbations, as well as in other spacetime theories. As a specific example, we consider here second-order perturbations in cosmology, assuming a flat Robertson - Walker background, giving explicit second-order transformations between the synchronous and the Poisson (generalized longitudinal) gauges.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Gauge-invariant cosmological perturbations
Bardeen, J. M. (1980) · Physical Review D · doi:10.1103/physrevd.22.1882 · Cited by 2,393
Does back reaction enforce the averaged null energy condition in semiclassical gravity?
Flanagan, E. E., & Wald, R. M. (1996) · Physical Review D · doi:10.1103/physrevd.54.6233 · Cited by 352
Cited by
Quasi-Normal Modes of Stars and Black Holes
Kokkotas, K. D., & Schmidt, B. G. (1999) · Living Reviews in Relativity · doi:10.12942/lrr-1999-2 · Cited by 2,055
A general proof of the conservation of the curvature perturbation
Lyth, D. H., Malik, K. A., & Sasaki, M. (2005) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2005/05/004 · Cited by 804
Teleparallel gravity: from theory to cosmology
Bahamonde, S., Dialektopoulos, K. F., Escamilla-Rivera, C., Farrugia, G., Gakis, V., Hendry, M., Hohmann, M., Levi Said, J., Mifsud, J., & Di Valentino, E. (2023) · Reports on Progress in Physics · doi:10.1088/1361-6633/ac9cef · Cited by 503
Energy-momentum tensor for cosmological perturbations
Abramo, L. R. W., Brandenberger, R. H., & Mukhanov, V. F. (1997) · Physical Review D · doi:10.1103/physrevd.56.3248 · Cited by 295
CMB polarization from secondary vector and tensor modes
Mollerach, S., Harari, D., & Matarrese, S. (2004) · Physical Review D · doi:10.1103/physrevd.69.063002 · Cited by 289
Self-citation
Metadata
- Authors
- Bruni, M., Matarrese, S., Mollerach, S., & Sonego, S.
- Venue
- Classical and Quantum Gravity
- Publisher
- IOP Publishing
- Published
- 1997-09-01
- Volume
- 14
- Issue
- 9
- Pages
- 2585-2606
- ISSN
- 0264-9381 (ISSN-L)
- 1361-6382
- OpenAlex
- W2061835457
- Cited by
- 343
- References
- 2
- FWCI
- 5.92
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond. https://app.cochat.ai/papers/10.1088/0264-9381/14/9/014
- The paper
- Bruni, M., Matarrese, S., Mollerach, S., & Sonego, S. (1997). Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/14/9/014
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.