In this work, the polarization contents of Einstein-\ae ther theory and theGeneralized T$e$V$e$S theory are discussed, as both theories have a normalizedtimelike vector field. The linearized equations of motion about the flatspacetime background are derived using the gauge invariant variables to easilyseparate physical degrees of freedom. The plane wave solutions are then found,and the polarizations are identified by examining the geodesic deviationequations. It shows that both theories contain six polarizations: plus, cross,vector-$x$, vector-$y$, transverse breathing and longitudinal polarizations. Wealso discuss the experimental tests of the extra polarizations in Einstein-\aether theory using pulsar timing arrays with the gravitational wave speed boundderived from the observations on GW 170817 and GRB 170817A. It turns out thatit is difficult to use pulsar timing arrays to distinguish differentpolarizations in Einstein-\ae ther theory. The same speed bound also forces oneof the propagating modes in the Generalized T$e$V$e$S theory to travel muchfaster than the speed of light, so the Generalized T$e$V$e$S theory isexcluded.
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机译:在本文中,讨论了爱因斯坦理论和广义T $ e $ V $ e $ S理论的极化内容,因为这两种理论都具有归一化的时态矢量场。使用规范不变变量可以轻松地分离物理自由度,从而得出关于平面时空背景的线性运动方程。然后找到平面波解,并通过检查测地线偏差方程来确定极化。它表明这两种理论都包含六个极化:加,交叉,矢量-$ x $,矢量-y $,横向呼吸和纵向极化。我们还讨论了使用脉冲星定时阵列以及从GW 170817和GRB 170817A的观测值推导出来的引力波速度对爱因斯坦-以太理论中的额外极化进行的实验测试。事实证明,在爱因斯坦理论中很难使用脉冲星定时阵列来区分不同的极化。相同的速度范围也迫使广义T $ e $ V $ e $ S理论中的一种传播模式比光速快得多,因此排除了广义T $ e $ V $ e $ S理论。
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