Gravitational wave (GW) polarizations are traditionally classified in a fixed frame ($E(2)$ classification), which does not account for how polarization patterns change under Lorentz boosts. In this work, we derive the explicit transformation laws for all six GW polarizations under longitudinal and transverse boosts. For gravity theories devoid of preferred frames, we propose a symmetry-based classification of the GW polarizations they admit. Among our key findings, we demonstrate that a propagating mode with five degrees of freedom strictly locks its longitudinal and breathing scalar amplitudes via the universal relation $A_l/A_b = -2(1-k^2/ω^2)$. For theories with a preferred frame, we analyze Bumblebee gravity and reveal that preferred-frame effects induce significant GW birefringence and observer-dependent polarization mixing. Crucially, we identify a novel vector-to-tensor polarization conversion mechanism, where vector modes in the preferred frame inevitably generate observable tensor polarizations for moving detectors, offering a new pathway to test Lorentz-violating gravity. Our framework provides a novel, observer-independent classification of GW polarizations and reveals previously unnoticed polarization mixing effects.
Testing for gravitationally preferred directions using the lunar orbit
由于引力是一种长程力,{ \it a priori}可以想象,宇宙的全球物质分布为局部引力物理学选择了一个优选的静止坐标系。在后牛顿近似下,偏好框架效应的现象学由两个参数描述,$α_1$和$α_2$,其中第二个参数已经受到非常严格的约束。重申以前的建议,我们通过一个详细的Hill-Brown型计算的扰动月球轨道,月球激光测距数据有可能约束$α_1$在$10^{-4}$水平。据发现,某些逆行平面轨道表现出共振敏感性的外部扰动链接到一个固定的方向在空间中。月球轨道离这样的共振很远,由于太阳潮汐,月球轨道没有明显的增强。我们的希尔-布朗分析扩展到与可能的差分加速度向银河系中心的扰动。然而,有人认为,有很强的{ \it先验}的理论约束,这种效果的可想象的大小。
Testing for Preferred-Frame Effects in Gravity with Artificial Earth Satellites
由于引力是一种长程力,人们可能会先验地期望宇宙的全球物质分布为局部引力物理学选择一个优选的静止框架。在后牛顿近似下,两个参数足以描述偏好框架效应的现象。其中一个已经被非常严格地限制(|alpha_2| < 4 x 10^-7,90% C. L),但另一种的结合力要弱得多(|alpha_1| < 5 x 10^-4,90% C. L.)。本文指出,观测人造地球卫星的特定轨道,由于小因子的出现,增强了相应的优选坐标系效应,有可能使α_1极限提高几个数量级。有一组离散的倾角,导致任意小的除数,而在零倾角(赤道)轨道中,地球静止轨道接近最佳。α_1引起的主要影响是:(一)轨道偏心率矢量的复杂长期演变,可描述为几个独立旋转的矢量和;和(二)卫星经度的年度振荡。
A Tighter Test of Local Lorentz Invariance using PSR J2317+1439
引力是一种长程力,人们可能{ \it a priori}期望宇宙的全球物质分布为局部引力物理学选择一个优选的静止框架。用两个参数$\hatα_1$和$\hatα_2$描述双星强引力场背景下的优选标架效应现象。这些参数在广义相对论中完全消失,并在弱场极限下简化为两个参数化后牛顿(PPN)参数$α_1$和$α_2$。我们导出了$|\hatα_1| < 1.7\times 10^{-4}$(90%~ C. L.)使用非常低的偏心率脉冲双星PSR J2317+1439,在以前的限制上提高了3倍。
Testing Local Lorentz Invariance with Laser Tracking of the LAGEOS and LAGEOS II Satellites
Istituto Nazionale di Astrofisica (INAF)(意大利国家天体物理研究所);Istituto di Astrofisica e Planetologia Spaziali (IAPS)(天体物理学与行星科学研究所);Istituto Nazionale di Fisica Nucleare (INFN)(意大利国家核物理研究所);Sezione di Tor Vergata(托尔维尔加塔分部);Consiglio Nazionale delle Ricerche (CNR)(意大利国家研究委员会);Istituto di Scienza e Tecnologie della Informazione (ISTI)(信息与科学技术研究所);Red de Infraestructuras Geodésicas, Instituto Geográfico Nacional(地理国家研究所大地测量基础设施网);Dipartimento di Fisica, Università di Tor Vergata(托尔维尔加塔大学物理系)