Gravitational Interaction of Spinning Bodies, Center-of-Mass Coordinate and Radiation of Compact Binary Systems
I.B. Khriplovich, A.A. Pomeransky

TL;DR
This paper analyzes spin-related gravitational effects in binary systems, proposing a new approach to defining the center-of-mass coordinate and revealing novel nonlinear spin effects in gravitational radiation.
Contribution
It introduces a new technique for treating spin effects in gravitational interactions and provides a corrected spin-orbit term differing from previous studies.
Findings
New definition of the center-of-mass coordinate.
Corrected spin-orbit interaction result.
Identification of nonlinear spin effects in gravitational radiation.
Abstract
Spin-orbit and spin-spin effects in the gravitational interaction are treated in a close analogy with the fine and hyperfine interactions in atoms. The proper definition of the cener-of-mass coordinate is discussed. The technique developed is applied then to the gravitational radiation of compact binary stars. Our result for the spin-orbit correction differs from that obtained by other authors. New effects possible for the motion of a spinning particle in a gravitational field are pointed out. The corresponding corrections, nonlinear in spin, are in principle of the same order of magnitude as the ordinary spin-spin interaction.
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