Parameter estimation for space-based gravitational wave detectors with ringdown signals
arXiv:2105.11279 · doi:10.1103/PhysRevD.104.083038
Abstract
Unlike ground-based gravitational wave detectors, space-based gravitational wave detectors can detect the ringdown signals from massive black hole mergers with large signal-to-noise ratios, help to localize sources and extract their parameters. To reduce the computation time in the Fisher information matrix analysis, we derive the analytical formulas of frequency-domain ringdown signals for both heliocentric and geocentric detectors by considering the effects of the harmonic phases, the rotation period of the geocentric detector, and the detector's arm length. We explore median errors of the parameter estimation and source localization with ringdown signals from binaries with different masses and different redshifts. Using a binary source with the total mass at the redshift , we analyze the dependence of these errors on the sky position. We find that the network of space-based gravitational wave detectors can significantly improve the source localization at the ringdown stage. The results of the Fisher matrix approximation are also checked by Bayesian inference method.
arXiv comment22 pages, 18 figures
References in corpus (81)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Advanced LIGO
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- TianQin: a space-borne gravitational wave detector
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- GW190521: A Binary Black Hole Merger with a Total Mass of
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- Interferometer design of the KAGRA gravitational wave detector
- Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
- On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
- Using gravitational-wave standard sirens
- GW150914: The Advanced LIGO Detectors in the Era of First Discoveries
- The construction and use of LISA sensitivity curves
- GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
- LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Measuring gravitational waves from binary black hole coalescences: I. Signal to noise for inspiral, merger, and ringdown
- Angular Resolution of the LISA Gravitational Wave Detector
- Inspiral, merger and ring-down of equal-mass black-hole binaries
- BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
- Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
- Rapid Bayesian position reconstruction for gravitational-wave transients
- Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits
- An improved effective-one-body Hamiltonian for spinning black-hole binaries
- Modeling Ringdown: Beyond the Fundamental Quasi-Normal Modes
- Predicting the direction of the final spin from the coalescence of two black holes
- LISA verification binaries with updated distances from Gaia Data Release 2
- The LISA-Taiji network
- Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
- Black-hole hair loss: learning about binary progenitors from ringdown signals
- Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era
- Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
- Black Hole Spectroscopy: Systematic Errors and Ringdown Energy Estimates
- Exploring the Bayesian parameter estimation of binary black holes with LISA
- Geometrical Expression for the Angular Resolution of a Network of Gravitational-Wave Detectors
- Higher signal harmonics, LISA's angular resolution, and dark energy
- Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
- Post-Newtonian accurate parametric solution to the dynamics of spinning compact binaries in eccentric orbits: The leading order spin-orbit interaction
- Is black-hole ringdown a memory of its progenitor?
- On the properties of the massive binary black hole merger GW170729
- Spectroscopic Evidence for a 5.4-Minute Orbital Period in HM Cancri
- RXJ0806.3+1527: a double degenerate binary with the shortest known orbital period (321s)
- Higher order gravitational-wave modes with likelihood reweighting
- Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals
- LISA observations of supermassive black holes: parameter estimation using full post-Newtonian inspiral waveforms
- Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
- Comparison of Gravitational Wave Detector Network Sky Localization Approximations
- The Angular Resolution of Space-Based Gravitational Wave Detectors
- Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
- Multi-mode black hole spectroscopy
- The Effect of Higher Harmonic Corrections on the Detection of massive black hole binaries with LISA
- LISA parameter estimation and source localization with higher harmonics of the ringdown
- GPU-accelerated massive black hole binary parameter estimation with LISA
- Parameter estimation for gravitational-wave bursts with the BayesWave pipeline
- Numerical simulation of sky localization for LISA-TAIJI joint observation
- Higher harmonics increase LISA's mass reach for supermassive black holes
- Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
- The LISA-Taiji network: precision localization of massive black hole binaries
- Realistic Event Rates for Detection of Supermassive Black Hole Coalescence by LISA
- Frequency response of space-based interferometric gravitational-wave detectors
- Localization of binary mergers with gravitational-wave detectors of second and third generation
- Black Hole Hunting with LISA
- Localization of transient gravitational wave sources: beyond triangulation
- Fisher vs. Bayes : A comparison of parameter estimation techniques for massive black hole binaries to high redshifts with eLISA
- Full analytical formulas for frequency response of space-based gravitational wave detectors
- LISA Source Confusion
- Sky localization of space-based gravitational wave detectors
- Frequency response of time-delay interferometry for space-based gravitational wave antennas
- Geometrical constraints upon the unipolar model of V407 Vul and RXJ0806.3+1527
- Swift X-ray and ultraviolet observations of the shortest orbital period double-degenerate system RX J0806.3+1527 (HM Cnc)
- Accuracy of estimation of parameters with space-borne gravitational wave observatory
- Fast localization of coalescing binaries with a heterogeneous network of advanced gravitational wave detectors