Disformal gravitational waves

Abstract Contrary to conformal transformations, disformal transformations can change the principal null directions of a spacetime geometry. Thus, depending on the frame a gravitational wave (GW) detector minimally couples to, the properties of GWs may change under a disformal transformation. In this paper, we provide necessary and sufficient conditions which determine whether GWs change under disformal transformations or not. Our argument is coordinate-independent and can be applied to any spacetime geometry at the fully non-linear level. As an example, we show that an exact radiative solution of massless Einstein-scalar gravity which admits only shear-free parallel transported frame is mapped to a disformed geometry which does not possess any shear-free parallel transported frame. This radiative geometry and its disformed counterpart provide a concrete example of the possibility to generate tensorial GWs from a disformal transformation at the fully non-linear level. This type of non-linear effect can be completely overlooked in the usual linear perturbation theory.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-02-01
DOI
https://doi.org/10.1088/1475-7516/2025/02/015
Citations
3
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.31
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article

Disformal gravitational waves

Jibril Ben Achour, Hugo Roussille, Mohammad Ali Gorji
3 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
2.31
article

Disformal gravitational waves

Jibril Ben Achour, Hugo Roussille, Mohammad Ali Gorji
article en
3 citations

Abstract

Abstract Contrary to conformal transformations, disformal transformations can change the principal null directions of a spacetime geometry. Thus, depending on the frame a gravitational wave (GW) detector minimally couples to, the properties of GWs may change under a disformal transformation. In this paper, we provide necessary and sufficient conditions which determine whether GWs change under disformal transformations or not. Our argument is coordinate-independent and can be applied to any spacetime geometry at the fully non-linear level. As an example, we show that an exact radiative solution of massless Einstein-scalar gravity which admits only shear-free parallel transported frame is mapped to a disformed geometry which does not possess any shear-free parallel transported frame. This radiative geometry and its disformed counterpart provide a concrete example of the possibility to generate tensorial GWs from a disformal transformation at the fully non-linear level. This type of non-linear effect can be completely overlooked in the usual linear perturbation theory.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(02)
École Normale Supérieure de Lyon (FR), Laboratoire de Physique de l'ENS de Lyon (FR)
Openalex Percentile: Top 13%
Cosmology and Gravitation Theories
2.31
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Disformal gravitational waves — Jibril Ben Achour, Hugo Roussille, et al. · Journal of Cosmology and Astroparticle Physics (2025) | TGRS Research Map | TGRS