Next-to-leading tail-induced spin-orbit effects in the gravitational radiation flux of compact binaries


The imprint of non-linearities in the propagation of gravitational waves — the tail effect — is responsible for new spin contributions to the energy flux and orbital phasing of spinning black hole binaries. The spin-orbit (linear in spin) contribution to this effect is currently known at leading post-Newtonian order, namely 3PN for maximally spinning black… (More)


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