Yu-Qi Dong, Xiao-Bin Lai, Yu-Qiang Liu, Yu-Xiao Liu
{"title":"Analyzing gravitational wave effects in general modified gravity: an example based on the most general vector-tensor theory","authors":"Yu-Qi Dong, Xiao-Bin Lai, Yu-Qiang Liu, Yu-Xiao Liu","doi":"arxiv-2409.11838","DOIUrl":null,"url":null,"abstract":"The Isaacson picture provides a general method for describing the effects of\ngravitational waves, established on two sets of basic equations. The first set\nof equations describes the propagation of gravitational waves within a given\nbackground, while the second set elucidates the interaction between the\neffective energy-momentum tensor of gravitational waves and the background\nmetric. These two sets of equations are typically derived by expanding the\nfield equations to second-order perturbations. In addition to the method of\nperturbing field equations, there is an alternative method: obtaining the two\nsets of basic equations by expanding the action to the second-order of\nperturbations. In this paper, we elaborate on this method, establishing its\nfoundations more rigorously. Especially, the second-order perturbation action,\nwith the Minkowski metric as the background, contains all necessary information\nto construct the Isaacson picture far from the source. We outline the\nderivation of the two sets of basic equations to describe the gravitational\nwave effects in the Isaacson picture, based on the second-order perturbation\naction. This will enable us to analyze the following effects: polarizations of\ngravitational waves, the wave speed for each polarization mode, the effective\nenergy-momentum tensor of gravitational waves, and the nonlinear memory effect\nof gravitational waves. We illustrate this method by applying it to the most\ngeneral second-order vector-tensor theory including parity-breaking terms. We\nfurther analyze the polarization modes of gravitational waves in this theory.\nWe highlight that this method facilitates model-independent research on various\ngravitational wave effects in general modified gravity theories. These effects\nare anticipated to be identified by the upcoming generation of gravitational\nwave detectors, aimed at testing potential modifications to gravity theory.","PeriodicalId":501339,"journal":{"name":"arXiv - PHYS - High Energy Physics - Theory","volume":"196 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - High Energy Physics - Theory","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11838","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
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.