Inference of the neutron star equation of state from cosmological distances
arXiv:2004.11334 · doi:10.1103/PhysRevLett.125.261101
Abstract
Finite-size effects on the gravitational wave signal from a neutron star merger typically manifest at high frequencies where detector sensitivity decreases. Proposed sensitivity improvements can give us access both to stronger signals and to a myriad of weak signals from cosmological distances. The latter will outnumber the former and the relevant part of signal will be redshifted towards the detector most sensitive band. We study the redshift dependence of information about neutron star matter and find that single-scale properties, such as the star radius or the post-merger frequency, are better measured from the distant weak sources from .
arXiv comment8 pages, 4 figures
References in corpus (113)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Astropy: A Community Python Package for Astronomy
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- A Massive Pulsar in a Compact Relativistic Binary
- Cosmic Star Formation History
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Advanced LIGO
- GW170817: Measurements of Neutron Star Radii and Equation of State
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
- Masses, Radii, and Equation of State of Neutron Stars
- Properties of the binary neutron star merger GW170817
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Science Case for the Einstein Telescope
- Equations of state for supernovae and compact stars
- Constraints on a phenomenologically parameterized neutron-star equation of state
- Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
- Gravitational-wave sensitivity curves
- Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
- Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Neutron-star radius constraints from GW170817 and future detections
- Binary neutron-star mergers: a review of Einstein's richest laboratory
- The mass ejection from the merger of binary neutron stars
- Towards gravitational-wave asteroseismology
- Identifying a first-order phase transition in neutron star mergers through gravitational waves
- Constraining the Equation of State with Moment of Inertia Measurements
- Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations
- Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing
- Measuring neutron-star properties via gravitational waves from binary mergers
- Merger of binary neutron stars with realistic equations of state in full general relativity
- Systematic parameter errors in inspiraling neutron star binaries
- Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
- Constraining the Equation of State of Neutron Stars from Binary Mergers
- Binary Neutron Star Mergers: Dependence on the Nuclear Equation of State
- Prompt merger collapse and the maximum mass of neutron stars
- Relativistic Numerical Method for Close Neutron Star Binaries
- Binary Neutron Star Mergers
- Modeling the complete gravitational wave spectrum of neutron star mergers
- Multi-messenger Bayesian parameter inference of a binary neutron-star merger
- Symmetry Energy I: Semi-Infinite Matter
- Search for post-merger gravitational waves from the remnant of the binary neutron star merger GW170817
- Systematic and statistical errors in a bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors
- Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state
- Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers
- Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
- Toward Early-Warning Detection of Gravitational Waves from Compact Binary Coalescence
- Testing Approximations of Thermal Effects in Neutron Star Merger Simulations
- Demonstrating the feasibility of probing the neutron star equation of state with second-generation gravitational wave detectors
- Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state
- GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
- Tidal deformability from GW170817 as a direct probe of the neutron star radius
- Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
- Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network
- Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects
- Reconstructing the neutron-star equation of state with gravitational-wave detectors from a realistic population of inspiralling binary neutron stars
- Gravitational waves and nonaxisymmetric oscillation modes in mergers of compact object binaries
- Observational constraints on hyperons in neutron stars
- Low mass binary neutron star mergers : gravitational waves and neutrino emission
- Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
- A Cryogenic Silicon Interferometer for Gravitational-wave Detection
- Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio
- Exploring properties of high-density matter through remnants of neutron-star mergers
- Gravitational waves from inspiraling compact binaries: Validity of the stationary-phase approximation to the Fourier transform
- Frequency-Dependent Squeezing for Advanced LIGO
- Constraining twin stars with GW170817
- Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence
- Unequal mass binary neutron star mergers and multimessenger signals
- Equation of state sensitivities when inferring neutron star and dense matter properties
- Unified treatment of sub-saturation stellar matter at zero and finite temperature
- Neutron-star Radius from a Population of Binary Neutron Star Mergers
- Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
- Tidal deformability with sharp phase transitions in (binary) neutron stars
- Conformally Flat Smoothed Particle Hydrodynamics: Application to Neutron Star Mergers
- Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves
- On the gravitational wave background from compact binary coalescences in the band of ground-based interferometers
- Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers
- Gravitational waves from relativistic neutron star mergers with nonzero-temperature equations of state
- Gravitational Radiation from Coalescing Binary Neutron Stars
- Inferring the post-merger gravitational wave emission from binary neutron star coalescences
- Metrics for next-generation gravitational-wave detectors
- Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signals
- Exploring the sensitivity of gravitational wave detectors to neutron star physics
- Binary Love Relations
- kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter
- Inferring neutron star properties from GW170817 with universal relations
- Observational Constraints on Neutron Star Masses and Radii
- Gravitational-Wave Asteroseismology with Fundamental Modes from Compact Binary Inspirals
- Causal Representations of Neutron-Star Equations of State
- Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors
- Studying strong phase transitions in neutron stars with gravitational waves
- Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
- From Neutron Star Observables to the Equation of State. I. An Optimal Parametrization
- Gravitational wave spectroscopy of binary neutron star merger remnants with mode stacking
- Cosmological inference using only gravitational wave observations of binary neutron stars
- Comparing two models for measuring the neutron star equation of state from gravitational-wave signals
- Modeling the postmerger gravitational wave signal and extracting binary properties from future binary neutron star detections
- Characteristics of hybrid compact stars with a sharp hadron-quark interface
- Host redshifts from gravitational-wave observations of binary neutron star mergers
- Waveform systematics for binary neutron star gravitational wave signals: effects of the point-particle baseline and tidal descriptions
- Relevance of tidal effects and post-merger dynamics for binary neutron star parameter estimation
- Equation of state effects and one-arm spiral instability in hypermassive neutron stars formed in eccentric neutron star mergers
- Constraining the p-mode--g-mode tidal instability with GW170817
- Second Einstein Telescope Mock Data and Science Challenge: Low Frequency Binary Neutron Star Data Analysis
- Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars
- Excitation of f-modes during mergers of spinning binary neutron star
- Joint search for isolated sources and an unresolved confusion background in pulsar timing array data
- Searching for exotic cores with binary neutron star inspirals
- Effect of squeezing on parameter estimation of gravitational waves emitted by compact binary systems
- Accelerated detection of the binary neutron star gravitational-wave background
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- Systematics of prompt black-hole formation in neutron star mergers
- Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass
- Uncertainty limits on neutron star radius measurements with gravitational waves
- Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
- 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
- Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
- Cosmography with next-generation gravitational wave detectors
- Astrophysical Implications of Neutron Star Inspiral and Coalescence
- Models of binary neutron star remnants with tabulated equations of state
- Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
- Prospects for Multimessenger Observations of Thorne-Żytkow Objects
- Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
- Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities
- Insights into Binary Neutron Star Merger Simulations: A Multi-Code Comparison
- Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
- Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
- Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
- Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences