Motion of a spinning particle under the conservative piece of the self-force is Hamiltonian to first order in mass and spin
arXiv:2302.10233 · doi:10.1103/PhysRevD.107.124017
Abstract
We consider the motion of a point particle with spin in a stationary spacetime. We define, following Witzany (2019) and later Ramond (2022), a twelve dimensional Hamiltonian dynamical system whose orbits coincide with the solutions of the Mathisson-Papapetrou-Dixon equations of motion with the Tulczyjew-Dixon spin supplementary condition, to linear order in spin. We then perturb this system by adding the conservative pieces of the leading order gravitational self-force and self-torque sourced by the particle's mass and spin. We show that this perturbed system is Hamiltonian and derive expressions for the Hamiltonian function and symplectic form. This result extends our previous result for spinless point particles.
arXiv comment7 pages
References in corpus (32)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- Binary Black Hole Mergers in the first Advanced LIGO Observing Run
- The motion of point particles in curved spacetime
- Gravitational Radiation Reaction to a Particle Motion
- An axiomatic approach to electromagnetic and gravitational radiation reaction of particles in curved spacetime
- Effective-one-body model for black-hole binaries with generic mass ratios and spins
- The Effective Field Theorist's Approach to Gravitational Dynamics
- Self-force and radiation reaction in general relativity
- Self-force via a Green's function decomposition
- Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory
- The International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background
- Effective Field Theories of Post-Newtonian Gravity: A comprehensive review
- Scattering Amplitudes and Conservative Binary Dynamics at
- Hamiltonian of a spinning test-particle in curved spacetime
- Second-order self-force calculation of the gravitational binding energy in compact binaries
- Second-order gravitational self-force
- Numerical Relativity and Astrophysics
- Hamiltonian formulation of general relativity and post-Newtonian dynamics of compact binaries
- Second Order Gravitational Self-Force
- Canonical Hamiltonian for an extended test body in curved spacetime: To quadratic order in spin
- Self-Force Calculations with a Spinning Secondary
- Investigating spinning test particles: spin supplementary conditions and the Hamiltonian formalism
- Hamiltonian Formulation of the Conservative Self-Force Dynamics in the Kerr Geometry
- Motion in classical field theories and the foundations of the self-force problem
- Hamiltonians and canonical coordinates for spinning particles in curved space-time
- A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
- The General Relativistic Two Body Problem and the Effective One Body Formalism
- Covariant hamiltonian spin dynamics in curved space-time
- Conservative second-order gravitational self-force on circular orbits and the effective one-body formalism
- Particle motion under the conservative piece of the self-force is Hamiltonian
- Spinning bodies in General Relativity
Cited by in corpus (7)
- Extreme mass-ratio inspiral and waveforms for a spinning body into a Kerr black hole via osculating geodesics and near-identity transformations
- Scattering and bound observables for spinning particles in Kerr spacetime with generic spin orientations
- Flux-balance laws for spinning bodies under the gravitational self-force
- Post-adiabatic waveform-generation framework for asymmetric precessing binaries
- Actions of spinning compact binaries: Spinning particle in Kerr matched to dynamics at 1.5 post-Newtonian order
- On the integrability of extended test body dynamics around black holes
- Gauss-Bonnet lensing of spinning massive particles in static spherically symmetric spacetimes