脉冲星引力洛伦兹破缺试验

Lijing Shao
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引用次数: 2

摘要

脉冲星是精确的天文时钟。当被放入二进制时,滴答声传达了潜在的时空几何动力学的秘密。我们使用脉冲星来测试引力相互作用是否与爱因斯坦的广义相对论(GR)有微小的偏差。在标准模型扩展(SME)的框架下,我们系统地搜索了由(a)质量维4的最小耦合、(b)质量维5的CPT对称和(c)质量维8的引力弱等效原理(GWEP)编目的违反洛伦兹算子。未发现GR偏差。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Pulsar Tests of Gravitational Lorentz Violation
Pulsars are precision celestial clocks. When being put in a binary, the ticking conveys the secret of underlying spacetime geometrodynamics. We use pulsars to test if the gravitational interaction possesses a tiny deviation from Einstein's General Relativity (GR). In the framework of Standard-Model Extension (SME), we systematically search for Lorentz-violating operators cataloged by (a) the minimal couplings of mass dimension 4, (b) the CPT symmetry of mass dimension 5, and (c) the gravitational weak equivalence principle (GWEP) of mass dimension 8. No deviation from GR was found yet.
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