Black hole spectroscopy for KAGRA future prospect in O5
arXiv:2003.06791 · doi:10.1103/PhysRevD.102.024007
Abstract
Ringdown gravitational waves of compact binary mergers are an important target to test general relativity. The main components of the ringdown waveform after merger are black hole quasinormal modes. In general relativity, all multipolar quasinormal modes of a black hole should give the same values of black hole parameters. Although the observed binary black hole events so far are not significant enough to perform the test with ringdown gravitational waves, it is expected that the test will be achieved in third generation detectors. The Japanese gravitational wave detector KAGRA, called bKAGRA for the current configuration, has started observation, and discussions for the future upgrade plans have also started. In this study, we consider which KAGRA upgrade plan is the best to detect the subdominant quasinormal modes of black holes in the aim of testing general relativity. We use a numerical relativity waveform as injected signals that contains two multipolar modes and analyze each mode by matched filtering. Our results suggest that the plan FDSQZ, which improves the sensitivity of KAGRA for broad frequency range, is the most suitable configuration for black hole spectroscopy.
References in corpus (45)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- 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
- Quasinormal modes of black holes and black branes
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- Tests of general relativity with GW150914
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- Binary Black Hole Mergers in the first Advanced LIGO Observing Run
- Interferometer design of the KAGRA gravitational wave detector
- On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
- Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
- Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework
- Inspiral, merger and ring-down of equal-mass black-hole binaries
- Black Hole Spectroscopy: Testing General Relativity through Gravitational Wave Observations
- Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
- Testing the no-hair theorem with GW150914
- A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem
- Black hole ringdown: the importance of overtones
- Matched-filtering and parameter estimation of ringdown waveforms
- Modeling Ringdown: Beyond the Fundamental Quasi-Normal Modes
- Observational Black Hole Spectroscopy: A time-domain multimode analysis of GW150914
- Bayesian model selection for testing the no-hair theorem with black hole ringdowns
- Mining information from binary black hole mergers: a comparison of estimation methods for complex exponentials in noise
- Black-hole hair loss: learning about binary progenitors from ringdown signals
- Testing the no-hair theorem with black hole ringdowns using TIGER
- Black-hole Spectroscopy by Making Full Use of Gravitational-Wave Modeling
- Ringdown overtones, black hole spectroscopy, and no-hair theorem tests
- Is black-hole ringdown a memory of its progenitor?
- The RIT binary black hole simulations catalog
- Empirical tests of the black hole no-hair conjecture using gravitational-wave observations
- Overtones or higher harmonics? Prospects for testing the no-hair theorem with gravitational wave detections
- Parametrized ringdown spin expansion coefficients: a data-analysis framework for black-hole spectroscopy with multiple events
- Post-Kerr black hole spectroscopy
- The next decade of black hole spectroscopy
- Decoding mode-mixing in black-hole merger ringdown
- Possible golden events for ringdown gravitational waves
- Comparison of various methods to extract ringdown frequency from gravitational wave data
- An Effective Search Method for Gravitational Ringing of Black Holes
- Estimation of starting times of quasinormal modes in ringdown gravitational waves with the Hilbert-Huang transform
- An Improved Search Method for Gravitational Ringing of Black Holes
- Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
- Measuring Spin of the Remnant Black Hole from Maximum Amplitude
- Parameterized and Consistency Tests of Gravity with Gravitational Waves: Current and Future
Cited by in corpus (6)
- Black hole spectroscopy horizons for current and future gravitational wave detectors
- Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
- Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory
- Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
- Fundamental Tone and Overtones of Quasinormal Modes in Ringdown Gravitational Waves: A Detailed Study in Black Hole Perturbation
- Universal horizons and black hole spectroscopy in gravitational theories with broken Lorentz symmetry