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Software . 2025
License: CC BY
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Software . 2025
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ZENODO
Software . 2025
License: CC BY
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ZENODO
Software . 2025
License: CC BY
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Radiated Angular Momentum from Spinning Black Hole Scattering Trajectories

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 25 Jun 2025Publisher:Zenodo
Authors: Mogull, Gustav; Plefka, Jan; Stoldt, Kathrin;

doi: 10.5281/zenodo.17792608 , 10.5281/zenodo.15740904 , 10.5281/zenodo.15740905

Radiated Angular Momentum from Spinning Black Hole Scattering Trajectories

Abstract

Ancillary file accompanying the paper "Radiated Angular Momentum from Spinning Black Hole Scattering Trajectories" submitted to arXiv.org and PRD providing all results for the spinning black hole trajectories, spin deflections and radiated angular momentum at leading order (1PM) and next-to-leading order (2PM) in the post-MInkowksian expansion inclduing up to quadratic in spin terms. v2: Error resulting from a wrong relative normalization in 2PM trajectory and spin kick corrected.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
Average
Average