Scope Out Multiband Gravitational-Wave Observations of GW190521-Like Binary Black Holes with Space Gravitational Wave Antenna B-DECIGO
Abstract
1. Introduction
Goals and Organization of This Paper
2. Method for Signal-to-Noise Ratio and Fisher Analysis
2.1. aLIGO, ET, B-DECIGO and LISA
2.2. Waveform Models
2.3. Signal-to-Noise Ratio
2.4. Multiband Fisher Analysis
3. Parameter Estimation Errors via Multiband Observation
3.1. Setup of Fisher Analysis
3.2. Result: Inspiral Phase
3.3. Result: Ringdown Phase
4. The Implications for Tests of GR via Multiband Observation
4.1. A Consistency test of GR with the Inspiral and Ringdown GW Signals
4.2. A Simple Test of the Remnant Compact Object with Quasinormal Modes
5. Summary and Discussion
Assessment of Prospects
Author Contributions
Funding
Informed Consent Statement
Data Availability Statement
Acknowledgments
Conflicts of Interest
Appendix A. Signal-to-Noise Ratio of GW190521-Like Eccentric BBH Systems
SNR and Eccentricity at | |||||
---|---|---|---|---|---|
aLIGO | |||||
ET | |||||
B-DECIGO | |||||
LISA | <1.00 | <1.00 | <1.00 | ||
(0.985) | (>0.999) | (>0.999) | (>0.999) |
Appendix B. Some More Noise Power Spectral Densities of (Next-Generation) GW Detectors
- “LIGO O3a-Livingston” rough fitting curve (during the first half of LIGO/Virgo third observing run by using Ref. [157]):
- “CE2” rough fitting curve (for Cosmic Explorer presented in Ref. [21]):
- “DECIGO” (the noise PSD of the L-shaped configuration [161]):
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Parameter | Symbol | |
---|---|---|
Primary mass [] | ||
Secondary mass [] | ||
Primary spin magnitude | ||
Secondary spin magnitude | ||
Total mass [] | ||
Mass ratio | ||
Luminosity Distance [Gpc] | ||
Redshift | z |
GW Detector | SNR | ||||
---|---|---|---|---|---|
BD + aLIGO | |||||
BD | |||||
aLIGO | ⋯ | ⋯ | ⋯ | ⋯ | |
BD + aLIGO | |||||
BD + ET | |||||
ET | ⋯ | ||||
BD + ET | |||||
LISA + BD + ET | |||||
LISA | ⋯ | ||||
LISA + BD | |||||
LISA + BD + ET |
GW Detector | SNR | ||
---|---|---|---|
aLIGO | |||
ET |
GW190521-Like BBH | GW150914-Like BBH | |||||
---|---|---|---|---|---|---|
GW Detector | SNR | SNR | ||||
Single band: Ringdown GW signal | ||||||
aLIGO | ||||||
ET | ||||||
Single band: inspiral GW signal | ||||||
BD | ||||||
Multiband: inspiral GW signal | ||||||
BD + ET | ||||||
LISA + BD | ||||||
LISA + BD + ET |
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Nakano, H.; Fujita, R.; Isoyama, S.; Sago, N. Scope Out Multiband Gravitational-Wave Observations of GW190521-Like Binary Black Holes with Space Gravitational Wave Antenna B-DECIGO. Universe 2021, 7, 53. https://doi.org/10.3390/universe7030053
Nakano H, Fujita R, Isoyama S, Sago N. Scope Out Multiband Gravitational-Wave Observations of GW190521-Like Binary Black Holes with Space Gravitational Wave Antenna B-DECIGO. Universe. 2021; 7(3):53. https://doi.org/10.3390/universe7030053
Chicago/Turabian StyleNakano, Hiroyuki, Ryuichi Fujita, Soichiro Isoyama, and Norichika Sago. 2021. "Scope Out Multiband Gravitational-Wave Observations of GW190521-Like Binary Black Holes with Space Gravitational Wave Antenna B-DECIGO" Universe 7, no. 3: 53. https://doi.org/10.3390/universe7030053
APA StyleNakano, H., Fujita, R., Isoyama, S., & Sago, N. (2021). Scope Out Multiband Gravitational-Wave Observations of GW190521-Like Binary Black Holes with Space Gravitational Wave Antenna B-DECIGO. Universe, 7(3), 53. https://doi.org/10.3390/universe7030053