Transverse-Traceless Gravitational Waves In A Spatially Flat FLRW Universe: Causal Structure from Dimension Reduction
Yi-Zen Chu

TL;DR
This paper explores how the causal structure of transverse-traceless gravitational waves in a flat FLRW universe can be understood through dimension reduction to 2D and 3D models, revealing tail effects and memory phenomena.
Contribution
It introduces a novel approach to analyze gravitational wave tails in FLRW universes via dimension reduction and exact solutions for power-law scale factors.
Findings
No TT gravitational wave tails in radiation-dominated universe
Tail amplitude is suppressed in matter-dominated universe
In de Sitter space, gravitational waves produce a memory effect
Abstract
This work was mainly driven by the desire to explore, to what extent embedding some given geometry in a higher dimensional flat one is useful for understanding the causal structure of classical fields traveling in the former, in terms of that in the latter. We point out, in the 4D spatially flat FLRW universe, that the causal structure of transverse-traceless (TT) gravitational waves can be elucidated by first reducing the problem to a 2D Minkowski wave equation with a time dependent potential, where the relevant Green's function is pure tail -- waves produced by a physical source propagate strictly within the null cone. By viewing this 2D world as embedded in a 4D one, the 2D Green's function can also be seen to be sourced by a cylindrically symmetric scalar field in 3D. From both the 2D wave equation as well as the 3D scalar perspective, we recover the exact solution of the 4D…
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