Theory of post-Newtonian radiation and reaction
arXiv:1305.6930 · doi:10.1103/PhysRevD.88.104037
Abstract
We address issues with extant formulations of dissipative effects in the effective field theory (EFT) which describes the post-Newtonian (PN) inspiral of two gravitating bodies by (re)formulating several parts of the theory. Novel ingredients include gauge invariant spherical fields in the radiation zone; a system zone which preserves time reversal such that its violation arises not from local odd propagation but rather from interaction with the radiation sector in a way which resembles the balayage method; 2-way multipoles to perform zone matching within the EFT action; and a double-field radiation-reaction action which is the non-quantum version of the Closed Time Path formalism and generalizes to any theory with directed propagators including theories which are defined by equations of motion rather than an action. This formulation unifies the treatment of outgoing radiation and its reaction force. We demonstrate the theory in the scalar, electromagnetic and gravitational cases by economizing the following: the expression for the radiation source multipoles; the derivation of the leading outgoing radiation and associated reaction force such that it is maximally reduced to mere multiplication; and the derivation of the gravitational next to leading PN order. In fact we present a novel expression for the +1PN correction to all mass multipoles. We introduce useful definitions for multi-index summation, for the normalization of Bessel functions and for the normalization of the gravito-magnetic vector potential.
v3: version published in Phys.Rev.D
References in corpus (16)
- The Hyperfine Einstein-Infeld-Hoffmann Potential
- The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
- Effective field theory calculation of second post-Newtonian binary dynamics
- The dynamics of the gravitational two-body problem at fourth post-Newtonian order and at quadratic order in the Newton constant
- Non-Relativistic Gravitation: From Newton to Einstein and Back
- Classical Effective Field Theory and Caged Black Holes
- Les Houches Lectures on Effective Field Theories and Gravitational Radiation
- The n-body problem in General Relativity up to the second post-Newtonian order from perturbative field theory
- An action for reaction in general dimension
- The Advanced LIGO Gravitational Wave Detector
- Gravitational radiation-reaction in arbitrary dimension
- Comment on `On the next-to-leading order gravitational spin(1)-spin(2) dynamics' by J. Steinhoff et al
- Dynamical vs. Auxiliary Fields in Gravitational Waves around a Black Hole
- Perturbations Around Backgrounds with One Non-Homogeneous Dimension
- Classical Effective Field Theory for Weak Ultra Relativistic Scattering
- Elementary development of the gravitational self-force
Cited by in corpus (14)
- Amplitudes, Observables, and Classical Scattering
- Effective Field Theories of Post-Newtonian Gravity: A comprehensive review
- Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
- Scalar QED as a toy model for higher-order effects in classical gravitational scattering
- Effective field theory for black holes with induced scalar charges
- Tests For Maximum Force and Maximum Power
- An action for reaction in general dimension
- Gravitational radiation-reaction in arbitrary dimension
- Analytic approximations, perturbation theory, effective field theory methods and their applications
- Classical 3-loop 2-body diagrams
- Radiation reaction at the level of the action
- Comments on initial conditions for the Abraham-Lorentz(-Dirac) equation
- Leading anomalies, the drift Hamiltonian and the relativistic two-body system
- Self force from equivalent periodic sources