More On Cosmological Gravitational Waves And Their Memories
Yi-Zen Chu

TL;DR
This paper extends theoretical understanding of gravitational wave propagation and memory effects in higher-dimensional FLRW universes, revealing scalar and tensor contributions, tail signals, and connections to gauge theories.
Contribution
It provides analytic expressions for graviton and photon Green's functions in higher-dimensional cosmologies, elucidates scalar and tensor wave contributions, and explores the gauge-invariant scalar mode and memory effects.
Findings
Scalar GWs can contribute to tidal effects around detectors.
Tail signals in certain cosmologies do not decay with distance.
A double copy relation links gravitational and Yang-Mills memory effects.
Abstract
We extend recent theoretical results on the propagation of linear gravitational waves (GWs), including their associated memories, in spatially flat Friedmann--Lema\^{i}tre--Robertson--Walker (FLRW) universes, for all spacetime dimensions higher than 3. By specializing to a cosmology driven by a perfect fluid with a constant equation-of-state -- conformal re-scaling, dimension-reduction and Nariai's ansatz may then be exploited to obtain analytic expressions for the graviton and photon Green's functions, allowing their causal structure to be elucidated. When , the gauge-invariant scalar mode admits wave solutions, and like its tensor counterpart, likely contributes to the tidal squeezing and stretching of the space around a GW detector. In addition, scalar GWs in 4D radiation dominated universes -- like tensor GWs in 4D matter dominated ones -- appear to yield a tail…
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