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.
Authors
- Jibril Ben Achour (ORCID: https://orcid.org/0000-0001-5796-2305)
- Hugo Roussille (ORCID: https://orcid.org/0000-0002-8407-1230)
- Mohammad Ali Gorji (ORCID: https://orcid.org/0000-0001-8848-2283)
Institutions
- École Normale Supérieure de Lyon (FR)
- Laboratoire de Physique de l'ENS de Lyon (FR)
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