Perturbative Frequency Expansion for Nearly Monochromatic Binary Black Holes Detectable with LISA
arXiv:2405.15999 · doi:10.1103/PhysRevD.110.023008
Abstract
The proposed space gravitational wave (GW) detector LISA has potential to detect stellar-mass black hole binaries (BBHs). The majority of the detected BBHs are expected to emit nearly monochromatic GWs, whose frequency evolution will be efficiently described by Taylor expansions. We study the measurability of the associated time derivative coefficients of the frequencies, by extending a recent work based on a simplified Fisher matrix analysis. Additionally, we provide qualitative discussions on how to extract astrophysical information, such as orbital eccentricity and tertiary perturbation, from the observed derivative coefficients.
arXiv comment11 pages, 6 figures, corrected Eq. (15) and related errors
References in corpus (30)
- TianQin: a space-borne gravitational wave detector
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- The construction and use of LISA sensitivity curves
- Taiji Program: Gravitational-Wave Sources
- Angular Resolution of the LISA Gravitational Wave Detector
- The promise of multi-band gravitational wave astronomy
- Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements
- Frequency and time domain inspiral templates for comparable mass compact binaries in eccentric orbits
- Multiband gravitational-wave event rates and stellar physics
- Parameter estimation for Galactic binaries by LISA
- Detecting hierarchical stellar systems with LISA
- The peculiar acceleration of stellar-origin black hole binaries: measurement and biases with LISA
- Binary radial velocity measurements with space-based gravitational-wave detectors
- PSR J1024-0719: A Millisecond Pulsar in an Unusual Long-Period Orbit
- A millisecond pulsar in an extremely wide binary system
- Listening to the gravitational wave sound of circumbinary exoplanets
- Long Term Operation of LISA and Galactic Close White Dwarf Binaries
- Evolution of binary systems accompanying axion clouds in extreme mass ratio inspirals
- Prospects of eLISA for Detecting Galactic Binary Black Holes Similar to GW150914
- Proposal for Determining the Total Masses of Eccentric Binaries Using Signature of Periastron Advance in Gravitational Waves
- Detecting Planets around Compact Binaries with Gravitational Wave Detectors in Space
- Two decades of optical timing of the shortest-period binary star system HM Cancri
- The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
- Degeneracy between mass and peculiar acceleration for the double white dwarfs in the LISA band
- How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
- Dynamics of Binary System around Supermassive Black Hole
- Tracking the Long-Term GW Phase Evolution for HM Cancri-like Binaries with LISA
- Potential Tertiary Effects on the LISA Verification Binary HM Cancri
- Forecasting Tidal Disruption Events by Binary Black Hole Roulettes