Next‐to‐next‐to‐leading order post‐Newtonian linear‐in‐spin binary Hamiltonians
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Publication:5300352
DOI10.1002/andp.201200271zbMath1269.83016arXiv1302.6723OpenAlexW1917850522WikidataQ114239030 ScholiaQ114239030MaRDI QIDQ5300352
Johannes Hartung, Jan Steinhoff, Gerhard Schäfer
Publication date: 27 June 2013
Published in: Annalen der Physik (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1302.6723
approximation methodsHamiltoniansequations of motionKerr spacetimepost-Newtonian approximationbinary starsADMcanonical formalismArnowitt-Deser-Misnerpost-Newtonian spin-orbit
Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (13)
Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order ⋮ The quadrupole moment of compact binaries to the fourth post-Newtonian order: I. Non-locality in time and infra-red divergencies ⋮ Post-Newtonian quasicircular initial orbits for numerical relativity ⋮ Gravitational quadratic-in-spin Hamiltonian at NNNLO in the post-Newtonian framework ⋮ Gravitational spin-orbit Hamiltonian at NNNLO in the post-Newtonian framework ⋮ Poincaré invariance of spinning binary dynamics in the post-Minkowskian Hamiltonian approach ⋮ The propagation delay in the timing of a pulsar orbiting a supermassive black hole ⋮ Analytic approximations, perturbation theory, effective field theory methods and their applications ⋮ The effective field theorist's approach to gravitational dynamics ⋮ The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem ⋮ Gravitational radiation from post-Newtonian sources and inspiralling compact binaries ⋮ Complete Hamiltonian for spinning binary systems at first post-Minkowskian order ⋮ Scattering of two spinning black holes in post-Minkowskian gravity, to all orders in spin, and effective-one-body mappings
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