pith. machine review for the scientific record. sign in

arxiv: gr-qc/9811047 · v1 · pith:IBAL54HSnew · submitted 1998-11-14 · 🌀 gr-qc · astro-ph· hep-th

Conformal transformations in classical gravitational theories and in cosmology

classification 🌀 gr-qc astro-phhep-th
keywords conformalframetheoriescosmologygravitationalclassicaleinsteingeneral
0
0 comments X
read the original abstract

In recent years, the use of conformal transformation techniques has become widespread in the literature on gravitational theories alternative to general relativity, on cosmology, and on nonminimally coupled scalar fields. Typically, the transformation to the Einstein frame is generated by a fundamental scalar field already present in the theory. In this context, the problem of which conformal frame is the physical one has to be dealt with and, in the general case, it has been clarified only recently; the formulation of a theory in the ``new'' conformal frame leads to departures from canonical Einstein gravity. In this article, we review the literature on conformal transformations in classical gravitational theories and in cosmology, seen both as purely mathematical tools and as maps with physically relevant aspects. It appears particularly urgent to refer the analysis of experimental tests of Brans-Dicke and scalar-tensor theories of gravity, as well as the predictions of cosmological inflationary scenarios, to the physical conformal frame, in order to have a meaningful comparison with the observations.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Could a so far ignored symmetry of the classical laws of gravity explain the cosmological puzzles?

    gr-qc 2025-10 unverdicted novelty 5.0

    Weyl symmetry of gravity is restored if masses transform as m → Ω^{-1}m under conformal changes, allowing any matter to couple invariantly and potentially accounting for dark energy and dark matter.

  2. Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion

    gr-qc 2026-04 unverdicted novelty 4.0

    In this two-field completion, trajectories connected to the Starobinsky solution keep entropy modes suppressed so that curvature and tensor perturbations remain effectively single-field Starobinsky-like.