Prospects for gravitational-wave observations of neutron-star tidal disruption in neutron-star/black-hole binaries
arXiv:gr-qc/9912026 · doi:10.1103/PhysRevLett.84.3519
Abstract
For an inspiraling neutron-star/black-hole binary (NS/BH), we estimate the gravity-wave frequency f_td at the onset of NS tidal disruption. We model the NS as a tidally distorted, homogeneous, Newtonian ellipsoid on a circular, equatorial geodesic around a Kerr BH. We find that f_td depends strongly on the NS radius R, and estimate that LIGO-II (ca. 2006-2008) might measure R to 15% precision at 140 Mpc (about 1 event/yr under current estimates). This suggests that LIGO-II might extract valuable information about the NS equation of state from tidal-disruption waves.
RevTeX, 4 pages, 2 EPS figures. Revised slightly, corrected typos
References in corpus (1)
Cited by in corpus (79)
- Tidal Love numbers of neutron stars
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach
- Effective One Body description of tidal effects in inspiralling compact binaries
- Numerical Relativity: A review
- Ergoregion instability of ultra-compact astrophysical objects
- Dynamical mass ejection from black hole-neutron star binaries
- Implications for the Origin of GRB 070201 from LIGO Observations
- Gravitational waves from spinning black hole-neutron star binaries: dependence on black hole spins and on neutron star equations of state
- Black hole-neutron star mergers at realistic mass ratios: Equation of state and spin orientation effects
- Extracting equation of state parameters from black hole-neutron star mergers. I. Nonspinning black holes
- Extracting equation of state parameters from black hole-neutron star mergers: aligned-spin black holes and a preliminary waveform model
- Equation of State Effects on Gravitational Waves from Rotating Core Collapse
- How Gravitational-wave Observations Can Shape the Gamma-ray Burst Paradigm
- Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves
- Merger of black hole-neutron star binaries in full general relativity
- Will black hole-neutron star binary inspirals tell us about the neutron star equation of state?
- Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3
- Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO
- Gravitational waves from black hole-neutron star binaries I: Classification of waveforms
- Gravitational waves from nonspinning black hole-neutron star binaries: dependence on equations of state
- Black hole-neutron star binary merger: Dependence on black hole spin orientation and equations of state
- Merger of black hole-neutron star binaries: nonspinning black hole case
- First-post-Newtonian quadrupole tidal interactions in binary systems
- Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
- Gravitomagnetic resonant excitation of Rossby modes in coalescing neutron star binaries
- Mergers of Magnetized Neutron Stars with Spinning Black Holes: Disruption, Accretion and Fallback
- The Science of the Einstein Telescope
- Probing neutron star superfluidity with gravitational-wave data
- Black hole tidal problem in the Fermi normal coordinates
- Numerical evolutions of a black hole-neutron star system in full General Relativity: I. Head-on collision
- Spectral Approach to the Relativistic Inverse Stellar Structure Problem II
- Measuring Neutron Star Radii with Gravitational Wave Detectors
- Implementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterparts
- Implications For The Origin Of GRB 051103 From LIGO Observations
- Gravitational-wave cutoff frequencies of tidally disruptive neutron star-black hole binary mergers
- Coalescence of black hole--neutron star binaries
- Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
- Mergers of Black Hole -- Neutron Star binaries. I. Methods and First Results
- Quasiequilibrium black hole-neutron star binaries in general relativity
- Black hole-neutron star binaries in general relativity: effects of neutron star spin
- Constraining the equation of state of nuclear matter with gravitational wave observations: Tidal deformability and tidal disruption
- Observing white dwarfs orbiting massive black holes in the gravitational wave and electro-magnetic window
- Neutron star tidal disruption in mixed binaries: the imprint of the equation of state
- Measuring precession in asymmetric compact binaries
- Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
- The Search for Gravitational Waves
- Quasiequilibrium sequences of black-hole--neutron-star binaries in general relativity
- Black Hole-Neutron Star Binaries in General Relativity: Quasiequilibrium Formulation
- Fermion-boson stars with a quartic self-interaction in the boson sector
- Nonspinning black hole-neutron star mergers: a model for the amplitude of gravitational waveforms
- Orbiting binary black hole evolutions with a multipatch high order finite-difference approach
- The Black Hole Remnant of Black Hole-Neutron Star Coalescing Binaries
- Inspiral of a Spinning Black Hole--Magnetized Neutron Star Binary: Increasing Charge and Electromagnetic Emission
- Learning about compact binary merger: the interplay between numerical relativity and gravitational-wave astronomy
- Black hole-neutron star mergers using a survey of finite-temperature equations of state
- On characteristic initial data for a star orbiting a black hole
- Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
- General-relativistic treatment of tidal -mode resonances in coalescing binaries of neutron stars. II. As triggers for precursor flares of short gamma-ray bursts
- Radio follow-up of gravitational wave triggers during Advanced LIGO O1
- Minimum energy and the end of the inspiral in the post-Newtonian approximation
- Black hole remnant of black hole-neutron star coalescing binaries with arbitrary black hole spin
- Tuning gravitational-wave detector networks to measure compact binary mergers
- Method to estimate ISCO and ring-down frequencies in binary systems and consequences for gravitational wave data analysis
- Constraining the Neutron Star Radius with Joint Gravitational-Wave and Short Gamma-Ray Burst Observations of Neutron Star-Black Hole Coalescing Binaries
- Gravitational waves from neutron star excitations in binary inspirals
- Multi-messenger Extended Emission from the compact remnant in GW170817
- Gravitational-wave astronomy: the high-frequency window
- Gravitational Wave Astronomy
- Are Post-Newtonian templates faithful and effectual in detecting gravitational signals from neutron star binaries?
- Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals II : Spectra for various cases
- Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals
- Gravitational waves from a dust disk around a Schwarzschild black hole
- Reconstructing the equation of state for cold nuclear matter from the relationship of any two properties of neutron stars
- Nuclear physics with gravitational waves from neutron stars disrupted by black holes
- Black hole-neutron star mergers with massive neutron stars in numerical relativity
- Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework
- Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
- On the frequency shift of gravitational waves