Journal
PHYSICAL REVIEW D
Volume 84, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.84.064041
Keywords
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Funding
- NSF [PHY-0903631]
- NASA [NNX09AI81G]
- CNRS
- Direct For Mathematical & Physical Scien
- Division Of Physics [903631] Funding Source: National Science Foundation
- NASA [115052, NNX09AI81G] Funding Source: Federal RePORTER
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Gravitational waves contain tail effects which are due to the backscattering of linear waves in the curved space-time geometry around the source. In this paper we improve the knowledge and accuracy of the two-body inspiraling post-Newtonian (PN) dynamics and gravitational-wave signal by computing the spin-orbit terms induced by tail effects. Notably, we derive those terms at 3PN order in the gravitational-wave energy flux, and 2.5PN and 3PN orders in the wave polarizations. This is then used to derive the spin-orbit tail effects in the phasing through 3PN order. Our results can be employed to carry out more accurate comparisons with numerical-relativity simulations and to improve the accuracy of analytical templates aimed at describing the whole process of inspiral, merger, and ringdown.
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