Comparing space+time decompositions in the post-Newtonian limit

DOI10.1088/0264-9381/28/14/145021zbMath1222.83155arXiv1011.6024OpenAlexW2140658892MaRDI QIDQ3091685

Barak Kol, Michael Smolkin, Michèle Levi

Publication date: 12 September 2011

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1011.6024

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (8)

Spinning gravitating objects in the effective field theory in the post-Newtonian scheme ⋮ A \(3+1\) formulation of the \(1/c\) expansion of general relativity ⋮ Holomorphic classical limit for spin effects in gravitational and electromagnetic scattering ⋮ \(\mathrm{N^3LO}\) spin-orbit interaction via the EFT of spinning gravitating objects ⋮ Classical effective field theory for weak ultra relativistic scattering ⋮ Amplitudes, observables, and classical scattering ⋮ Gravitational cubic-in-spin interaction at the next-to-leading post-Newtonian order ⋮ Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics

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