Constraining three-nucleon forces with multimessenger data
arXiv:2010.03581 · doi:10.1103/PhysRevC.103.065804
Abstract
We report the results of a study aimed at inferring direct information on the repulsive three-nucleon potential \textemdash driving the stiffness of the nuclear matter equation of state at supranuclear densities\textemdash from astrophysical observations. Using a Bayesian approach, we exploit the measurements of masses, radii and tidal deformabalities performed by the NICER satellite and the LIGO/Virgo collaboration, as well as the mass of the heaviest observed pulsar, to constrain the strength of . The baseline of our analysis is the widely employed nuclear Hamiltonian comprising the Argonne nucleon-nucleon potential andthe Urbana IX model of three-nucleon potential. The numerical results, largely determined by the bound on the maximum mass, suggest that existing and future facilities have the potential to provide valuable new insight into microscopic nuclear dynamics at supranuclear densities.
arXiv commentDiscussion of the results extended. Various changes to match the version in press on Phys. Rev. C
References in corpus (66)
- emcee: The MCMC Hammer
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- An accurate nucleon-nucleon potential with charge-independence breaking
- The equation of state for nucleon matter and neutron star structure
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
- Determination of the Equation of State of Dense Matter
- Tidal Love numbers of neutron stars
- Properties of the binary neutron star merger GW170817
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Science Case for the Einstein Telescope
- SparsePak: A Formatted Fiber Field Unit for The WIYN Telescope Bench Spectrograph. I. Design, Construction, and Calibration
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- The Equation of State from Observed Masses and Radii of Neutron Stars
- Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
- Relativistic tidal properties of neutron stars
- Quantum Monte Carlo methods for nuclear physics
- Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
- Relativistic theory of tidal Love numbers
- New constraints on radii and tidal deformabilities of neutron stars from GW170817
- Evidence for quark-matter cores in massive neutron stars
- The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars
- Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817
- Constraints on the density dependence of the symmetry energy
- GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
- Neutron-star radius constraints from GW170817 and future detections
- KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
- Astrophysical Measurement of the Equation of State of Neutron Star Matter
- Constraining the neutron-proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density
- Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
- Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
- Neutron star tidal deformability and equation of state constraints
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
- Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
- GW190814: Impact of a 2.6 solar mass neutron star on nucleonic equations of state
- Neutron star tidal deformabilities constrained by nuclear theory and experiment
- Constraining the symmetry energy at subsaturation densities using isotope binding energy difference and neutron skin thickness
- A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star
- Astrophysical and theoretical physics implications from multimessenger neutron star observations
- Constraints on the Skyrme Equations of State from Properties of Doubly Magic Nuclei
- Direct Astrophysical Tests of Chiral Effective Field Theory at Supranuclear Densities
- Constraining the equation of state of high-density cold matter using nuclear and astronomical measurements
- First-post-Newtonian quadrupole tidal interactions in binary systems
- New class of hybrid EoS and Bayesian M-R data analysis
- On the nature of GW190814 and its impact on the understanding of supranuclear matter
- Inferring neutron star properties from GW170817 with universal relations
- The mass and the radius of the neutron star in the transient low mass X-ray binary SAX J1748.9-2021
- Constraining nuclear matter parameters with GW170817
- Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements
- Constraining the neutron star equation of state using multi-band independent measurements of radii and tidal deformabilities
- Shear viscosity of neutron matter from realistic nucleon-nucleon interactions
- GW190814: On the properties of the secondary component of the binary
- Multi-messenger and multi-physics Bayesian inference for GW170817 binary neutron star merger
- Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
- Microscopic calculations of transport properties of neutron matter
- Neutral current interactions of low-energy neutrinos in dense neutron matter
- Correlation effects on the weak response of nuclear matter
- Tidal Deformation of Neutron Stars from Microscopic Models of Nuclear Dynamics
- Superfluid Gap in Neutron Matter from a Microscopic Effective Interaction
- Scale Dependence of Nucleon-Nucleon Potentials
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- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Modelling frequency-dependent tidal deformability for environmental black-hole mergers
- Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
- Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
- Measuring tidal effects with the Einstein Telescope: A design study
- Tidal Love numbers and approximate universal relations for fermion soliton stars
- Bayesian inference of neutron-skin thickness and neutron-star observables based on effective nuclear interactions
- Testing the Paradigm of Nuclear Many-Body Theory
- Inferring three-nucleon couplings from multi-messenger neutron-star observations
- Modeling Neutron Star Matter in the Age of Multimessenger Astrophysics
- Shell quenching in nuclear charge radii based on Monte Carlo dropout Bayesian neural network
- Relativistic Corrections to the CBF Effective Nuclear Hamiltonian
- Spacetime curvature corrections for the Yukawa potential and its application for the Reissner-Nordström Metric
- Impact and detectability of spin-tidal couplings in neutron star inspirals
- Constraining Hamiltonians from chiral effective field theory with neutron-star data
- Impact of three-nucleon forces on gravitational wave emission from neutron stars