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Non-Relativistic Gravitation: From Newton to Einstein and Back

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arxiv 0712.4116 v3 pith:MXMXDIMZ submitted 2007-12-26 hep-th gr-qc

Non-Relativistic Gravitation: From Newton to Einstein and Back

classification hep-th gr-qc
keywords correctionpotentialcorrespondingfieldgravito-magneticinteractionnon-relativisticvector
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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.

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