Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order

Abstract

The gravitational radiation from point particle binaries is computed at the third post-Newtonian (3PN) approximation of general relativity. Three previously introduced ambiguity parameters, coming from the Hadamard self-field regularization of the 3PN source-type mass quadrupole moment, are consistently determined by means of dimensional regularization, and proved to have the values xi = -9871/9240, kappa = 0 and zeta = -7/33. These results complete the derivation of the general relativistic prediction for compact binary inspiral up to 3.5PN order, and should be of use for searching and deciphering the signals in the current network of gravitational wave detectors.

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References in corpus (34)

• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian order
• The Last Three Minutes: Issues in Gravitational Wave Measurements of Coalescing Compact Binaries
• Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
• Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order
• Gravitational radiation from compact binary systems: gravitational waveforms and energy loss to second post-Newtonian order
• Improved filters for gravitational waves from inspiralling compact binaries
• Dimensional regularization of the gravitational interaction of point masses
• Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit
• Gravitational-Wave Inspiral of Compact Binary Systems to 7/2 Post-Newtonian Order
• Gravitational waves from inspiralling compact binaries: Energy loss and waveform to second--post-Newtonian order
• 3rd post-Newtonian higher order Hamilton dynamics for two-body point-mass systems
• Testing gravity to second post-Newtonian order: a field-theory approach
• Dimensional regularization of the third post-Newtonian dynamics of point particles in harmonic coordinates
• Third post-Newtonian dynamics of compact binaries: Noetherian conserved quantities and equivalence between the harmonic-coordinate and ADM-Hamiltonian formalisms
• General relativistic dynamics of compact binaries at the third post-Newtonian order
• Gravitational waves from inspiralling compact binaries: Energy flux to third post-Newtonian order
• Poincaré invariance in the ADM Hamiltonian approach to the general relativistic two-body problem
• The 2.5PN gravitational wave polarisations from inspiralling compact binaries in circular orbits
• Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case
• Gravitational-wave tails of tails
• Energy losses by gravitational radiation in inspiralling compact binaries to five halves post-Newtonian order
• Equivalence between the ADM-Hamiltonian and the harmonic-coordinates approaches to the third post-Newtonian dynamics of compact binaries
• Second-post-Newtonian generation of gravitational radiation
• On the multipole expansion of the gravitational field
• Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries
• New derivation of a third post-Newtonian equation of motion for relativistic compact binaries without ambiguity
• The binary black-hole problem at the third post-Newtonian approximation in the orbital motion: Static part
• On the equations of motion of point-particle binaries at the third post-Newtonian order
• Gravitational radiation from a particle in circular orbit around a black hole. VI. Accuracy of the post-Newtonian expansion
• On Estimation of the Post-Newtonian Parameters in the Gravitational-Wave Emission of a Coalescing Binary
• Equation of motion for relativistic compact binaries with the strong field point particle limit: Third post-Newtonian order
• Equation of motion for relativistic compact binaries with the strong field point particle limit : the second and half post-Newtonian order
• Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates

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