Analyzing gravitational wave effects in general modified gravity: an example based on the most general vector-tensor theory

Yu-Qi Dong, Xiao-Bin Lai, Yu-Qiang Liu, Yu-Xiao Liu
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Abstract

The Isaacson picture provides a general method for describing the effects of gravitational waves, established on two sets of basic equations. The first set of equations describes the propagation of gravitational waves within a given background, while the second set elucidates the interaction between the effective energy-momentum tensor of gravitational waves and the background metric. These two sets of equations are typically derived by expanding the field equations to second-order perturbations. In addition to the method of perturbing field equations, there is an alternative method: obtaining the two sets of basic equations by expanding the action to the second-order of perturbations. In this paper, we elaborate on this method, establishing its foundations more rigorously. Especially, the second-order perturbation action, with the Minkowski metric as the background, contains all necessary information to construct the Isaacson picture far from the source. We outline the derivation of the two sets of basic equations to describe the gravitational wave effects in the Isaacson picture, based on the second-order perturbation action. This will enable us to analyze the following effects: polarizations of gravitational waves, the wave speed for each polarization mode, the effective energy-momentum tensor of gravitational waves, and the nonlinear memory effect of gravitational waves. We illustrate this method by applying it to the most general second-order vector-tensor theory including parity-breaking terms. We further analyze the polarization modes of gravitational waves in this theory. We highlight that this method facilitates model-independent research on various gravitational wave effects in general modified gravity theories. These effects are anticipated to be identified by the upcoming generation of gravitational wave detectors, aimed at testing potential modifications to gravity theory.
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分析广义修正引力中的引力波效应:基于最广义矢量张量理论的实例
艾萨克森图提供了一种描述引力波效应的一般方法,它建立在两组基本方程之上。第一组方程描述了引力波在给定背景中的传播,而第二组方程则阐明了引力波的有效能动张量与背景度量之间的相互作用。这两组方程通常是通过将场方程扩展到二阶扰动而得到的。除了扰动场方程的方法之外,还有另一种方法:通过将作用扩展到二阶扰动来获得两组基本方程。在本文中,我们详细阐述了这一方法,更严格地建立了它的基础。特别是以明考斯基度量为背景的二阶扰动作用,包含了构建远离源的艾萨克森图景的所有必要信息。我们概述了基于二阶扰动作用的两组基本方程的衍生,以描述艾萨克森图景中的引力波效应。这将使我们能够分析以下效应:引力波的极化、每种极化模式的波速、引力波的有效能量-动量张量以及引力波的非线性记忆效应。我们将这一方法应用于最一般的二阶矢量张量理论,包括奇偶性破坏项,以此来说明这一方法。我们进一步分析了该理论中的引力波极化模式。我们强调,这种方法有助于在一般修正引力理论中开展与模型无关的各种引力波效应研究。这些效应预计将被即将问世的引力波探测器识别出来,以测试对引力理论的潜在修正。
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