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• W2730002806 abstract "We show initial data for gravitational axial waves that are twice differentiable but that are not ${C}^{2}$. They generate wave pulses that interact with matter in the radiation cosmological era. This forces the radiation matter to rotate. This rotation is permanent---it persists after the passage of the gravitational pulse. The observed inhomogeneities of the cosmic microwave background radiation put a bound onto discontinuities of superhorizon metric perturbations. We explicitly show that a class of smooth initial metrics that are at least ${C}^{2}$ gives rise to gravitational wave pulses that do not interact with the background during the radiation epoch." @default.
• W2730002806 created "2017-07-14" @default.
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• W2730002806 date "2017-09-26" @default.
• W2730002806 modified "2023-10-09" @default.
• W2730002806 title "Axial gravitational waves in FLRW cosmology and memory effects" @default.
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• W2730002806 doi "https://doi.org/10.1103/physrevd.96.063523" @default.
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