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}
}
  • A. Antonelli, M. Meent, +2 authors Justin Vines
  • Published 2019
  • Physics
  • arXiv: General Relativity and Quantum Cosmology
  • 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

    Figures and Tables from this paper.

    References

    Publications referenced by this paper.
    SHOWING 1-10 OF 171 REFERENCES