# Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information

@article{Antonelli2019QuasicircularIA, title={Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information}, author={A. Antonelli and M. Meent and A. Buonanno and J. Steinhoff and Justin Vines}, journal={arXiv: General Relativity and Quantum Cosmology}, year={2019} }

The self-force program aims at accurately modeling relativistic two-body systems with a small mass ratio (SMR). In the context of the effective-one-body (EOB) framework, current results from this program can be used to determine the effective metric components at linear order in the mass ratio, resumming post-Newtonian (PN) dynamics around the test-particle limit in the process. It was shown in [Akcay et al., Phys. Rev. D 86 (2012)] that, in the original (standard) EOB gauge, the SMR… CONTINUE READING

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