论文标题
深色能量引力波
Gravitational Waves with Dark Energy
论文作者
论文摘要
在本文中，我们研究了在非零-LAMBDA作为暗能量的情况下扰动的张量模式方程，其动态性质取决于哈勃参数H和/或其时间派生词。根据总真空贡献，暗能量在辐射主导的时代具有轻微的效果，但在物质统治时代进入地平线的波长中，重力波（GWS）的平方幅度最高为60％。
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.
