Completing the fifth PN precision frontier via the EFT of spinning gravitating objects

DOI10.1007/JHEP04(2023)079arXiv2211.14018OpenAlexW4366421524MaRDI QIDQ6105649

Zhewei Yin, Michèle Levi

Publication date: 9 June 2023

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2211.14018

zbMATH Keywords

scattering amplitudesblack holesspace-time symmetrieseffective field theories

Mathematics Subject Classification ID

Quantum theory (81-XX)

Related Items (6)

Spin Supplementary condition in quantum field theory: covariant SSC and physical state projection ⋮ From the EFT of spinning gravitating objects to Poincaré and gauge invariance at the 4.5PN precision frontier ⋮ Recursion in the classical limit and the neutron-star Compton amplitude ⋮ \(\mathrm{N^3LO}\) spin-orbit interaction via the EFT of spinning gravitating objects ⋮ Scattering in black hole backgrounds and higher-spin amplitudes. II. ⋮ Poincaré invariance of spinning binary dynamics in the post-Minkowskian Hamiltonian approach

Cites Work

• Testing binary dynamics in gravity at the sixth post-Newtonian level
• Gravitational cubic-in-spin interaction at the next-to-leading post-Newtonian order
• On the vanishing of Love numbers for Kerr black holes
• Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics
• The fifth-order post-newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach: potential contributions
• The 6th post-Newtonian potential terms at \(O( G_N^4)\)
• Scattering of spinning black holes from exponentiated soft factors
• Black hole stereotyping: induced gravito-static polarization
• Spinning gravitating objects in the effective field theory in the post-Newtonian scheme
• The 2PM Hamiltonian for binary Kerr to quartic in spin
• Love symmetry
• A tale of tails through generalized unitarity
• Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order
• Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
• Gravitational spin-orbit Hamiltonian at NNNLO in the post-Newtonian framework

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