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arXiv 0712.4116hep-thgr-qc
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非相对论引力:从牛顿到爱因斯坦再回来

Non-Relativistic Gravitation: From Newton to Einstein and Back

Barak Kol, Michael Smolkin

摘要:

我们提出了一个改进的经典有效理论方法的非相对论或后牛顿近似的广义相对论。“势度规场”通过时间Kaluza-Klein变换分解为三个NRG场:一个与牛顿势相同的标量场、一个与重磁矢量势对应的3-矢量场和一个3-张量场。爱因斯坦-因菲尔德-霍夫曼拉格朗日量的推导简化了,使得每一项对应于一个费曼图,提供了一个清晰的物理解释。自旋相互作用主要由重力-磁场的交换决定。给出了自旋-自旋相互作用的3 PN修正和自旋-轨道相互作用的2.5PN修正对应的主修正图。

英文摘要:

We present an improvement to the Classical Effective Theory approach to the non-relativistic or Post-Newtonian approximation of General Relativity. The "potential metric field" is decomposed through a temporal Kaluza-Klein ansatz into three NRG-fields: a scalar identified with the Newtonian potential, a 3-vector corresponding to the gravito-magnetic vector potential and a 3-tensor. The derivation of the Einstein-Infeld-Hoffmann Lagrangian simplifies such that each term corresponds to a single Feynman diagram providing a clear physical interpretation. Spin interactions are dominated by the exchange of the gravito-magnetic field. Leading correction diagrams corresponding to the 3PN correction to the spin-spin interaction and the 2.5PN correction to the spin-orbit interaction are presented.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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