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Solar System Tests of the Equivalence Principle and Constraints on Higher-Dimensional Gravity

机译:等效重力原理和约束的太阳系测试

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摘要

In most studies of equivalence principle violation by solar system bodies, it is assumed that the ratio of gravitational to inertial mass for a given body deviates from unity by a parameter Delta which is proportional to its gravitational self-energy. Here we inquire what experimental constraints can be set on Delta for various solar system objects when this assumption is relaxed. Extending an analysis originally due to Nordtvedt, we obtain upper limits on linearly independent combinations of Delta for two or more bodies from Kepler's third law, the position of Lagrange libration points, and the phenomenon of orbital polarization. Combining our results, we extract numerical upper bounds on Delta for the Sun, Moon, Earth and Jupiter, using observational data on their orbits as well as those of the Trojan asteroids. These are applied as a test case to the theory of higher-dimensional (Kaluza-Klein) gravity. The results are three to six orders of magnitude stronger than previous constraints on the theory, confirming earlier suggestions that extra dimensions play a negligible role in solar systemdynamics and reinforcing the value of equivalence principle tests as a probe of nonstandard gravitational theories.
机译:在大多数太阳系天体违反等价原理的研究中,假设给定天体的重力质量与惯性质量之比偏离单位为Δ的参数Delta与其重力自能成正比。在此,我们可以放宽这个假设,可以为各种太阳系物体在Delta上设置哪些实验约束。扩展最初由Nordtvedt引起的分析,我们从开普勒第三定律,拉格朗日解放点的位置以及轨道极化现象中获得了两个或多个物体的Delta线性独立组合的上限。结合我们的结果,我们使用太阳系,木星系和特洛伊木星系的轨道观测数据,提取了太阳,月亮,地球和木星的Delta数值上限。这些作为测试案例应用于高维(Kaluza-Klein)重力理论。结果比以前对该理论的约束要强三到六个数量级,这证实了先前的建议,即额外尺寸在太阳系动力学中起着微不足道的作用,并加强了等效原理测试的价值,以此作为非标准引力理论的探究。

著录项

  • 作者

    Overduin, J M;

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  • 年度 2000
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  • 原文格式 PDF
  • 正文语种 eng
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