Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
arXiv:2004.02527 · doi:10.1007/s10714-020-02751-6
Abstract
Gravitational waves emitted from the coalescence of neutron star binaries open a new window to probe matter and fundamental physics in unexplored, extreme regimes. To extract information about the supranuclear matter inside neutron stars and the properties of the compact binary systems, robust theoretical prescriptions are required. We give an overview about general features of the dynamics and the gravitational wave signal during the binary neutron star coalescence. We briefly describe existing analytical and numerical approaches to investigate the highly dynamical, strong-field region during the merger. We review existing waveform approximants and discuss properties and possible advantages and shortcomings of individual waveform models, and their application for real gravitational-wave data analysis.
arXiv commentinvited review for General Relativity and Gravitation; any comment or suggestion is welcome
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- Evolution of Highly Eccentric Binary Neutron Stars Including Tidal Effects
- Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
- Black hole evolution with the BSSN system by pseudo-spectral methods
- iResum: a new paradigm for resumming gravitational wave amplitudes
- Strangeons constitute bulk strong matter-- To test using GW170817
- Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state
- Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
- Convective Excitation of Inertial Modes in Binary Neutron Star Mergers
- Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. II: the higher multipolar modes
- Numerical Relativity Simulations of Precessing Binary Neutron Star Mergers
- Long term black hole evolution with the BSSN system by pseudospectral methods
- Impact of Numerical Relativity information on effective-one-body waveform models
- Gravitational wave extraction based on Cauchy-characteristic extraction and characteristic evolution
- Constraining the observer angle of the kilonova AT2017gfo associated with GW170817: Implications for the Hubble constant
- Radiation Magnetohydrodynamics for Black Hole-Torus System in Full General Relativity: A Step toward Physical Simulation
- Second post-Newtonian order radiative dynamics of inspiralling compact binaries in the Effective Field Theory approach
- Linear-in-mass-ratio contribution to spin precession and tidal invariants in Schwarzschild spacetime at very high post-Newtonian order
- Horizon-absorbed energy flux in circularized, nonspinning black-hole binaries and its effective-one-body representation
- Gravitomagnetic tidal effects in gravitational waves from neutron star binaries
- A post-Newtonian diagnosis of quasiequilibrium configurations of neutron star-neutron star and neutron star-black hole binaries
- Initial data for binary neutron stars with adjustable eccentricity
- Effects of nuclear symmetry energy and equation of state on neutron star properties
- Tidal deformation of a slowly rotating material body: Interior metric and Love numbers
- The General Relativistic Two Body Problem and the Effective One Body Formalism
- Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
- Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
- From micro to macro and back: probing near-horizon quantum structures with gravitational waves
- Upper limit set by causality on the tidal deformability of a neutron star
- Finite tidal effects in GW170817: Observational evidence or model assumptions?
- Waveform systematics for binary neutron star gravitational wave signals: Effects of spin, precession, and the observation of electromagnetic counterparts
- Tidal deformations of neutron stars: The role of stratification and elasticity
- Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars
- Excitation of f-modes during mergers of spinning binary neutron star
- Constraint to chiral invariant masses of nucleons from GW170817 in an extended parity doublet model
- Compact objects in scalar-tensor theories after GW170817
- Nonspinning black hole-neutron star mergers: a model for the amplitude of gravitational waveforms
- Probing the high-density behavior of symmetry energy with gravitational waves
- Quasi-5.5PN TaylorF2 approximant for compact binaries: point-mass phasing and impact on the tidal polarizability inference
- Spectral Cauchy Characteristic Extraction of strain, news and gravitational radiation flux
- Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. III: the spinning test-body terms
- Future Prospects for Constraining Nuclear Matter Parameters with Gravitational Waves
- Initial data for neutron star binaries with arbitrary spins
- Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
- Dynamical response to a stationary tidal field
- Rotating neutron stars with non-barotropic thermal profile
- On the validity of the adiabatic approximation in compact binary inspirals
- Exploring strong-field deviations from general relativity via gravitational waves
- Stability of nonspinning effective-one-body model in approximating two-body dynamics and gravitational-wave emission
- I-Love relation for incompressible stars and realistic stars
- Effect of spin on the inspiral of binary neutron stars
- Empirical constraints on the high-density equation of state from multi-messenger observables
- Inspiralling eccentric binary neutron stars: orbital motion and tidal resonance
- I-Love-Q Relations for Neutron Stars in dynamical Chern Simons Gravity
- Gravitational waveforms for neutron star binaries from binary black hole simulations
- Impact of high spins on the ejection of mass in GW170817
- Are neutron stars crushed? Gravitomagnetic tidal fields as a mechanism for binary-induced collapse
- Tidal Effects in Eccentric Coalescing Neutron Star Binaries
- Tidal interaction in compact binaries: a post-Newtonian affine framework
- Consistent Skyrme parametrizations constrained by GW170817
- General-relativistic coupling between orbital motion and internal degrees of freedom for inspiraling binary neutron stars
- The nonspinning binary black hole merger scenario revisited
- Octupolar invariants for compact binaries on quasi-circular orbits
- Two-layer compact stars with crystalline quark matter: Screening effect on the tidal deformability
- Extended I-Love relations for slowly rotating neutron stars
- Role of crustal physics in the tidal deformation of a neutron star
- Universal Relations and Alternative Gravity Theories
- Hadron matter in neutron stars in view of gravitational wave observations
- Unified description of astrophysical properties of neutron stars independent of the equation of state
- Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling for two nonprecessing black holes with aligned spins
- Conservative second-order gravitational self-force on circular orbits and the effective one-body formalism
- Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the spin orientation
- Universality and stationarity of the I-Love relation for self-bound stars
- Role of the crust on the tidal deformability of a neutron star within a unified treatment of dense matter
- Geometric polarization of plasmas and Love numbers of AdS black branes
- GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
- An accurate metric for the spacetime around neutron stars
- Theory of post-Newtonian radiation and reaction
- An effective field theory approach to tidal dynamics of spinning astrophysical systems
- Solving the relativistic inverse stellar problem through gravitational waves observation of binary neutron stars
- Dense matter equation of state for neutron star mergers
- Relativistic tidal properties of superfluid neutron stars
- Tidal Deformability of Neutron Stars with Realistic Nuclear Energy Density Functionals
- Initial-data contribution to the error budget of gravitational waves from neutron-star binaries
- Compact Star of Holographic Nuclear Matter and GW170817
- Gravitational waves from neutron star excitations in binary inspirals
- Completion of the universal I-Love-Q relations in compact stars including the mass
- Implications of the fermion vacuum term in the extended SU(3) Quark Meson model on compact stars properties
- Neutron star equation of state and GW170817
- The heavier the better: how to constrain mass ratios and spins of high-mass neutron-star mergers
- A variational formalism for tidal excitation: non-rotating, homentropic stars
- Constraints on Skyrme Equations of State from Doubly Magic Nuclei, Ab-Initio Calculations of Low-Density Neutron Matter, and Neutron Stars
- Properties of binary components and remnant in GW170817 using equations of state in finite temperature field theory models
- Covariant Equations of Motion of Extended Bodies with Arbitrary Mass and Spin Multipoles
- Constructing Love-Q-Relations with Gravitational Wave Detections
- Properties of strange quark stars with isovector interactions
- Inverse Structure Problem for Neutron-Star Binaries
- Gravitational-wave-driven tidal secular instability in neutron star binaries
- Effect of superfluid matter of neutron star on the tidal deformability
- Tidal invariants along the world line of an extended body in the Kerr spacetime
- Forecasting Gamma-Ray Bursts using Gravitational Waves
- Dynamical evolution and leading order gravitational wave emission of Riemann-S binaries
- Radiation reaction at the level of the action
- Three little pieces for computer and relativity
- Constraints on the Neutron Star Equation of State from GW170817
Cited by in corpus (72)
- Science-Driven Tunable Design of Cosmic Explorer Detectors
- Leading Nonlinear Tidal Effects and Scattering Amplitudes
- The Science of the Einstein Telescope
- Merger and post-merger of binary neutron stars with a quark-hadron crossover equation of state
- Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
- Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
- The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
- Modelling frequency-dependent tidal deformability for environmental black-hole mergers
- Uncertainty limits on neutron star radius measurements with gravitational waves
- Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
- Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity
- Bayesian inference of strange star equation of state using the GW170817 and GW190425 data
- Gravitational Bremsstrahlung with tidal effects in the post-Minkowskian expansion
- Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
- Frequency deviations in universal relations of isolated neutron stars and postmerger remnants
- Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
- Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
- Holographic approach to compact stars and their binary mergers
- Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
- Implementation of Monte-Carlo transport in the general relativistic SpEC code
- A fast radio burst with sub-millisecond quasi-periodic structure
- Can fermion-boson stars reconcile multi-messenger observations of compact stars?
- Radial pulsations, moment of inertia and tidal deformability of dark energy stars
- Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
- Impact of pions on binary neutron star mergers
- Thermal behavior as indicator for hyperons in binary neutron star merger remnants
- Measuring tidal effects with the Einstein Telescope: A design study
- Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
- Applications of machine learning in gravitational wave research with current interferometric detectors
- Neutron star mass-radius constraints using the high-frequency QPOs of GRB 200415A
- Tidal Love numbers and approximate universal relations for fermion soliton stars
- High-accuracy simulations of highly spinning binary neutron star systems
- Models of binary neutron star remnants with tabulated equations of state
- Probing horizon scale quantum effects with Love
- New gravitational waveform model for precessing binary neutron stars with double-spin effects
- -mode Imprints in Gravitational Waves from Coalescing Binaries involving Aligned Spinning Neutron Stars
- Reverse phase transitions in binary neutron-star systems with exotic-matter cores
- Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
- Geodesic structure and quasinormal modes of a tidally perturbed spacetime
- Multipole tidal effects in the post-Newtonian gravitational-wave phase of compact binary coalescences
- Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
- Effects of Onset of Phase Transition on Binary Neutron Star Mergers
- Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations
- Premerger phenomena in neutron-star binary coalescences
- Gravitational wave emission from dynamical stellar interactions
- High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
- Hidden symmetry between rotational tidal Love numbers of spinning neutron stars
- Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
- Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
- Thermal effects on tidal deformability in the last orbits of an inspiraling binary neutron star system
- Nonparametric extensions of nuclear equations of state: probing the breakdown scale of relativistic mean-field theory
- Simulating neutron stars with a flexible enthalpy-based equation of state parametrization in SpECTRE
- Validating Sequential Monte Carlo for Gravitational-Wave Inference
- Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
- High-energy neutrino signatures from pulsar remnants of binary neutron-star mergers: coincident detection prospects with gravitational waves
- Gravitational-wave searches in the era of Advanced LIGO and Virgo
- Dark energy effects on realistic neutron stars
- First Law of Mechanics for Spinning Compact Binaries: Dipolar Order
- Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
- Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
- Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
- Gravitational-wave model for neutron star merger remnants with supervised learning
- Insights into Binary Neutron Star Merger Simulations: A Multi-Code Comparison
- Role of particle diffusion in shaping the gravitational wave signal from neutron star inspirals
- Phenomenological Implications of a Magnetic 5th Force
- Machine learning-driven conservative-to-primitive conversion in hybrid piecewise polytropic and tabulated equations of state
- Binary black holes in the heat of merger
- Gamma-radiation sky maps from compact binaries
- Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
- Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
- Impact of Higher-order Tidal Corrections on the Measurement Accuracy of Neutron Star Tidal Deformability
- Updated estimates of post-merger gravitational wave energy released in GW170817 and the maximum neutron star mass