Nonlocal-in-time effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
arXiv:2301.01070 · doi:10.1103/PhysRevD.107.084018
Abstract
We complete the nonlocal-in-time effective-one-body (EOB) formalism of conservative dynamics for massless Scalar-Tensor (ST) theories at third post-Newtonian (PN) order. The nonlocal-in-time EOB Hamiltonian is obtained by mapping the order-reduced Hamiltonian corresponding to the nonlocal-in-time Lagrangian derived in [Phys. Rev. D 99, 044047 (2019)]. To transcribe the dynamics within EOB formalism, we use a strategy of order-reduction of nonlocal dynamics to local ordinary action-angle Hamiltonian. We then map this onto the EOB Hamiltonian to determine the nonlocal-in-time ST corrections to the EOB potentials at 3PN order.
8 Pages
References in corpus (14)
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory
- Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
- Fourth post-Newtonian effective one-body dynamics
- Energy and periastron advance of compact binaries on circular orbits at the fourth post-Newtonian order
- Compact binary systems in scalar-tensor gravity. III. Scalar waves and energy flux
- Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits
- Gravitational waves in scalar-tensor theory to one-and-a-half post-Newtonian order
- Dynamics of compact binary systems in scalar-tensor theories: II. Center-of-mass and conserved quantities to 3PN order
- Spin-orbit effects for compact binaries in scalar-tensor gravity
- Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
- Effective-action model for dynamical scalarization beyond the adiabatic approximation
- Tensor-Multi-Scalar Gravity: Equations of Motion to 2.5 post-Newtonian Order
- Relativistic effects in a mildly recycled pulsar binary: PSR J1952+2630
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