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Post Newtonian emission of gravitational waves from binary systems: a gauge theory perspective

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arxiv 2311.14637 v3 pith:VA6C336B submitted 2023-11-24 gr-qc hep-th

classification gr-qchep-th
keywords binaryformgaugegravitationalnewtonianorderpostsystems
verification ladder T0 review T1 audit T2 compute T3 formal
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We derive a gauge inspired combinatorial formula based on localization for the Post-Newtonian expansion of the gravitational wave form luminosity of binary systems made of objects with very different masses orbiting at large distances and small velocities. The results are tested against previous formulae in the literature for Schwarschild and Kerr black holes at the 5th and 3rd Post Newtonian order respectively beyond the quadrupole approximation. Tidal effects show up in the wave form at the 5th PN order, providing a quantitative measure of the blackness/compactness properties of the heavy object.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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