Gravitational Waves with Dark Energy
arXiv:2208.06844 · doi:10.1016/j.jheap.2022.07.003
Abstract
In this article, we study the tensor mode equation of perturbation in the presence of nonzero-Lambda as dark energy, the dynamic nature of which depends on the Hubble parameter H and/or its time derivative. Dark energy, according to the total vacuum contribution, has a slight effect during the radiation-dominated era, but it reduces the squared amplitude of gravitational waves (GWs) up to 60% for the wavelengths that enter the horizon during the matter-dominated era.
arXiv comment19 pages, 3 Figure
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