Next-to-next-to-leading order gravitational spin-squared potential via the effective field theory for spinning objects in the post-Newtonian scheme
Mich\`ele Levi, Jan Steinhoff

TL;DR
This paper derives the next-to-next-to-leading order spin-squared interaction potential for compact binaries using effective field theory in the post-Newtonian framework, advancing the precision of gravitational modeling for spinning objects.
Contribution
It provides the first derivation of the spin-squared potential at this order, including all relevant Feynman diagrams, within the effective field theory approach.
Findings
Complete spin-squared potential at 4PN order for spinning binaries.
All Feynman diagrams and their values are provided.
Demonstrates robustness of EFT for spinning gravitating objects.
Abstract
The next-to-next-to-leading order spin-squared interaction potential for generic compact binaries is derived for the first time via the effective field theory for gravitating spinning objects in the post-Newtonian scheme. The spin-squared sector is an intricate one, as it requires the consideration of the point particle action beyond minimal coupling, and mainly involves the spin-squared worldline couplings, which are quite complex, compared to the worldline couplings from the minimal coupling part of the action. This sector also involves the linear in spin couplings, as we go up in the nonlinearity of the interaction, and in the loop order. Hence, there is an excessive increase in the number of Feynman diagrams, of which more are higher loop ones. We provide all the Feynman diagrams and their values. The beneficial nonrelativistic gravitational fields are employed in the computation.…
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