A comparison of search templates for gravitational waves from binary inspiral - 3.5PN update
arXiv:gr-qc/0207021 · doi:10.1103/PhysRevD.66.027502
Abstract
Phasing formulas in a recent paper of ours' (Phys. Rev. D 63, 044023-1 (2001) are updated taking into account the recent 3.5PN results. Some misprints in the published version of the recent paper are also corrected.
eta-dependent tail terms have been corrected in view of related Errata by Blanchet and Iyer (2005)
Cited by in corpus (62)
- Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
- Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
- Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
- High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions
- Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
- Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
- Transition from inspiral to plunge in precessing binaries of spinning black holes
- Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit
- Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state
- LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
- Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
- Phasing of gravitational waves from inspiralling eccentric binaries
- Where post-Newtonian and numerical-relativity waveforms meet
- A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case
- Testing post-Newtonian theory with gravitational wave observations
- Ready-to-use post-Newtonian gravitational waveforms for binary black holes with non-precessing spins: An update
- High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
- Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era
- Probing Planckian corrections at the horizon scale with LISA binaries
- Higher signal harmonics, LISA's angular resolution, and dark energy
- Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
- The binary black-hole dynamics at the third-and-a-half post-Newtonian order in the ADM-formalism
- Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms
- Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates
- Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
- A quasi-physical family of gravity-wave templates for precessing binaries of spinning compact objects: Application to double-spin precessing binaries
- Accuracy and effectualness of closed-form, frequency-domain waveforms for non-spinning black hole binaries
- Probing General Relativity With Mergers of Supermassive and Intermediate-Mass Black Holes
- Suitability of post-Newtonian/numerical-relativity hybrid waveforms for gravitational wave detectors
- Statistical and systematic errors for gravitational-wave inspiral signals: A principal component analysis
- Impact of high-order tidal terms on binary neutron-star waveforms
- Waveform accuracy and systematic uncertainties in current gravitational wave observations
- Testing the multipole structure of compact binaries using gravitational wave observations
- Parameter estimation on compact binary coalescences with abruptly terminating gravitational waveforms
- Improving gravitational-wave parameter estimation using Gaussian process regression
- Reliability of complete gravitational waveform models for compact binary coalescences
- Accuracy of binary black hole waveform models for aligned-spin binaries
- Are Parametrized Tests of General Relativity with Gravitational Waves Robust to Unknown Higher Post-Newtonian Order Effects?
- Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
- Gravitational-wave detectors as particle-physics laboratories: Constraining scalar interactions with a coherent inspiral model of boson-star binaries
- Mergers of Irrotational Neutron Star Binaries in Conformally Flat Gravity
- Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
- Generic bounds on dipolar gravitational radiation from inspiralling compact binaries
- Singular value decomposition in parametrised tests of post-Newtonian theory
- Superposed metric for spinning black hole binaries approaching merger
- Gravitational waveforms for neutron star binaries from binary black hole simulations
- Application of asymptotic expansions of maximum likelihood estimators errors to gravitational waves from binary mergers: the single interferometer case
- Parameter estimation of coalescing supermassive black hole binaries with LISA
- Synergy of short gamma ray burst and gravitational wave observations: Constraining the inclination angle of the binary and possible implications for off-axis gamma ray bursts
- Ineffectiveness of Padé resummation techniques in post-Newtonian approximations
- Post-Newtonian templates for gravitational waves from compact binary inspirals
- New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test-mass in the Schwarzschild spacetime
- Improving the efficiency of the detection of gravitational wave signals from inspiraling compact binaries: Chebyshev interpolation
- A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
- Comparison of post-Newtonian templates for extreme mass ratio inspirals
- Probe for Type Ia supernova progenitor in decihertz gravitational wave astronomy
- Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
- On the approximate relation between black-hole perturbation theory and numerical relativity
- Gravitational and electromagnetic emission by magnetized coalescing binary systems
- Searching for gravitational waves emitted by binaries with spinning components