Leading-order gravitational radiation to all spin orders
Abstract
Starting with on-shell amplitudes compatible with the scattering of Kerr black holes up to Compton-amplitude contact terms, we produce the gravitational waveform and memory effect including spin at their leading post-Minkowskian orders to all orders in the spins of both scattering objects. For the memory effect, we present results at next-to-leading order as well, finding a closed form for all spin orders when the spins are anti-aligned and equal in magnitude. Considering instead generically oriented spins, we produce the next-to-leading-order memory to sixth order in spin. Compton-amplitude contact terms up to sixth order in spin are included throughout our analysis.
Copyright and License
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
Funding
Funded by SCOAP3.
Acknowledgement
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Additional details
- ISSN
- 2470-0029
- UCLouvain
- Knut and Alice Wallenberg Foundation
- KAW 2018.0116
- Knut and Alice Wallenberg Foundation
- KAW 2018.0162
- UK Research and Innovation
- European Commission
- EP/X037312/1
- United States Department of Energy
- DE-SC0011632
- California Institute of Technology
- Walter Burke Institute for Theoretical Physics
- Caltech groups
- Walter Burke Institute for Theoretical Physics