Abstract
The effective one-body theories, introduced by Buonanno and Damour, are novel approaches to constructing a gravitational waveform template. By taking a gauge in which ψ B1 and ψ B3 vanish, we find a decoupled equation with separable variables for ψ B4 in the effective metric obtained in the post-Minkowskian approximation. Furthermore, we set up a new self-consistent effective one-body theory for spinless binaries, which can be applicable to any post-Minkowskian orders. This theory not only releases the assumption that v/c should be a small quantity but also resolves the contradiction that the Hamiltonian, radiation-reaction force, and waveform are constructed from different physical models in the effective one-body theory with the post-Newtonian approximation. Compared with our previous theory [Sci. China-Phys. Mech. Astron. 65, 260411 (2022)], the computational effort for the radiation-reaction force and waveform in this new theory will be tremendously reduced.
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This work was supported by the National Natural Science Foundation of China (Grant Nos. 12035005, 12122504, and 11875025), and National Key Research and Development Program of China (Grant No. 2020YFC2201400). We would like to thank professors S. Chen and Q. Pan for useful discussions on the manuscript.
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Jing, J., Long, S., Deng, W. et al. New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation. Sci. China Phys. Mech. Astron. 65, 100411 (2022). https://doi.org/10.1007/s11433-022-1951-1
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DOI: https://doi.org/10.1007/s11433-022-1951-1