Some Gravity Waves in Isotropic Cosmologies
Peter A. Hogan, Dirk Puetzfeld

TL;DR
This paper constructs and analyzes non-planar gravitational wave solutions in isotropic expanding universes, showing their effects on matter content and providing both perturbative and exact models.
Contribution
It introduces new non-planar gravitational wave models in isotropic cosmologies, linking perturbative and exact solutions with matter content modifications.
Findings
Gravitational waves cause anisotropic stress in the universe.
Wave front expansion is driven solely by cosmic expansion.
Perturbative and exact models align under certain approximations.
Abstract
We construct metric perturbations of two families of isotropic expanding universes describing gravitational waves propagating through these universes. The waves are non--planar and owe their wave front expansion solely to the expansion of the universes. The presence of this radiation leads to a small perturbation of the perfect fluid matter content of the universes by the appearance of an anisotropic stress. We then construct exact models of gravity waves in these universes. In this case the matter content of the models consists of the perfect fluid matter supplemented by anisotropic stress and lightlike matter traveling with the waves. Under appropriate conditions of approximation the lightlike matter can be neglected and the exact models coincide with the perturbative models.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
