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Title: Constraining nuclear matter parameters with GW170817

Abstract

The tidal measurement of gravitational waves from the binary neutron star merger event GW170817 allows us to probe nuclear physics that suffers less from astrophysical systematics compared to neutron star radius measurements with electromagnetic wave observations. Recent research found strong correlation among neutron-star tidal deformabilities and certain combinations of nuclear parameters associated with the equation of state. These relations were then used to derive bounds on such parameters from GW170817 assuming that the relations and neutron star masses are known exactly. In this work, we expand on this important work by taking into account a few new considerations: (1) a broader class of equations of state; (2) correlations with the mass-weighted tidal deformability that was directly measured with GW170817; (3) how the relations depend on the binary mass ratio; (4) the uncertainty from equation of state variation in the correlation relations; (5) adopting the updated posterior distribution of the tidal deformability measurement from GW170817. Upon these new considerations, we find GW170817 90% confidence intervals on nuclear parameters (the incompressibility K0, its slope M0, and the curvature of symmetry energy Ksym,0 at nuclear saturation density) to be 81 MeV ≤K0 ≤362 MeV, 1556 MeV ≤M0 ≤ 4971 MeV, and -259 MeVmore » ≤Ksym, 0 ≤32 MeV, which are more conservative than previously found with systematic errors more properly taken into account.« less

Authors:
 [1];  [2];  [1]
  1. Univ. of Virginia, Charlottesville, VA (United States)
  2. Univ. of Tennessee, Knoxville, TN (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
Publication Date:
Research Org.:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP)
OSTI Identifier:
1505302
Alternate Identifier(s):
OSTI ID: 1546145
Grant/Contract Number:  
AC05-00OR22725
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review D
Additional Journal Information:
Journal Volume: 99; Journal Issue: 4; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Carson, Zack, Steiner, Andrew W., and Yagi, Kent. Constraining nuclear matter parameters with GW170817. United States: N. p., 2019. Web. doi:10.1103/PhysRevD.99.043010.
Carson, Zack, Steiner, Andrew W., & Yagi, Kent. Constraining nuclear matter parameters with GW170817. United States. https://doi.org/10.1103/PhysRevD.99.043010
Carson, Zack, Steiner, Andrew W., and Yagi, Kent. Wed . "Constraining nuclear matter parameters with GW170817". United States. https://doi.org/10.1103/PhysRevD.99.043010. https://www.osti.gov/servlets/purl/1505302.
@article{osti_1505302,
title = {Constraining nuclear matter parameters with GW170817},
author = {Carson, Zack and Steiner, Andrew W. and Yagi, Kent},
abstractNote = {The tidal measurement of gravitational waves from the binary neutron star merger event GW170817 allows us to probe nuclear physics that suffers less from astrophysical systematics compared to neutron star radius measurements with electromagnetic wave observations. Recent research found strong correlation among neutron-star tidal deformabilities and certain combinations of nuclear parameters associated with the equation of state. These relations were then used to derive bounds on such parameters from GW170817 assuming that the relations and neutron star masses are known exactly. In this work, we expand on this important work by taking into account a few new considerations: (1) a broader class of equations of state; (2) correlations with the mass-weighted tidal deformability that was directly measured with GW170817; (3) how the relations depend on the binary mass ratio; (4) the uncertainty from equation of state variation in the correlation relations; (5) adopting the updated posterior distribution of the tidal deformability measurement from GW170817. Upon these new considerations, we find GW170817 90% confidence intervals on nuclear parameters (the incompressibility K0, its slope M0, and the curvature of symmetry energy Ksym,0 at nuclear saturation density) to be 81 MeV ≤K0 ≤362 MeV, 1556 MeV ≤M0 ≤ 4971 MeV, and -259 MeV ≤Ksym, 0 ≤32 MeV, which are more conservative than previously found with systematic errors more properly taken into account.},
doi = {10.1103/PhysRevD.99.043010},
journal = {Physical Review D},
number = 4,
volume = 99,
place = {United States},
year = {Wed Feb 20 00:00:00 EST 2019},
month = {Wed Feb 20 00:00:00 EST 2019}
}

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Cited by: 58 works
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Works referenced in this record:

Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817
journal, August 2018


Binary Love relations
journal, June 2016


Skyrme force and the mass formula
journal, February 1976


New Constraints on Radii and Tidal Deformabilities of Neutron Stars from GW170817
journal, June 2018


Neutron Star Tidal Deformabilities Constrained by Nuclear Theory and Experiment
journal, August 2018


Maximum mass of neutron stars and strange neutron-star cores
journal, February 2013


Spectral representations of neutron-star equations of state
journal, November 2010


Equations of state for supernovae and compact stars
journal, March 2017


Masses, Radii, and the Equation of State of Neutron Stars
journal, September 2016


GW170817: Measurements of Neutron Star Radii and Equation of State
journal, October 2018


Mass and radius formulas for low-mass neutron stars
journal, May 2014

  • Sotani, H.; Iida, K.; Oyamatsu, K.
  • Progress of Theoretical and Experimental Physics, Vol. 2014, Issue 5
  • DOI: 10.1093/ptep/ptu052

Spectral approach to the relativistic inverse stellar structure problem II
journal, March 2014


Symmetry Parameter Constraints from a Lower Bound on Neutron-matter Energy
journal, October 2017

  • Tews, Ingo; Lattimer, James M.; Ohnishi, Akira
  • The Astrophysical Journal, Vol. 848, Issue 2
  • DOI: 10.3847/1538-4357/aa8db9

Equation of state for dense nucleonic matter from metamodeling. II. Predictions for neutron star properties
journal, February 2018

  • Margueron, Jérôme; Hoffmann Casali, Rudiney; Gulminelli, Francesca
  • Physical Review C, Vol. 97, Issue 2
  • DOI: 10.1103/PhysRevC.97.025806

Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models
journal, September 2003


Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State
journal, April 2018


On the Lorentz structure of the symmetry energy
journal, February 2004


The Equation of State from Observed Masses and Radii of Neutron Stars
journal, September 2010

  • Steiner, Andrew W.; Lattimer, James M.; Brown, Edward F.
  • The Astrophysical Journal, Vol. 722, Issue 1
  • DOI: 10.1088/0004-637X/722/1/33

Erratum: Spectral approach to the relativistic inverse stellar structure problem. II [Phys. Rev. D 89 , 064003 (2014)]
journal, June 2016


Spectral approach to the relativistic inverse stellar structure problem
journal, October 2012


A unified equation of state of dense matter and neutron star structure
journal, December 2001


Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII. Stiffness and stability of neutron-star matter
journal, September 2010


Relativistic mean field calculations with density-dependent meson-nucleon coupling
journal, September 1999


Determination of the parameters of a Skyrme type effective interaction using the simulated annealing approach
journal, July 2005


Density dependence of the nuclear symmetry energy: A microscopic perspective
journal, October 2009


Tidal deformabilities and neutron star mergers
journal, September 2018


Low‐Mass Neutron Stars and the Equation of State of Dense Matter
journal, August 2003

  • Carriere, J.; Horowitz, C. J.; Piekarewicz, J.
  • The Astrophysical Journal, Vol. 593, Issue 1
  • DOI: 10.1086/376515

GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
journal, January 2018

  • Radice, David; Perego, Albino; Zappa, Francesco
  • The Astrophysical Journal, Vol. 852, Issue 2
  • DOI: 10.3847/2041-8213/aaa402

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
journal, October 2017


Approximate universal relations among tidal parameters for neutron star binaries
journal, December 2016


Relativistic mean-field theory for unstable nuclei with non-linear σ and ω terms
journal, October 1994


Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
journal, April 2016

  • Silva, Hector O.; Sotani, Hajime; Berti, Emanuele
  • Monthly Notices of the Royal Astronomical Society, Vol. 459, Issue 4
  • DOI: 10.1093/mnras/stw969

Nuclear effective forces and isotope shifts
journal, February 1995


Interdependence of different symmetry energy elements
journal, August 2017


Composition and thermodynamics of nuclear matter with light clusters
journal, January 2010


Tidal Love Numbers of Neutron Stars
journal, April 2008

  • Hinderer, Tanja
  • The Astrophysical Journal, Vol. 677, Issue 2
  • DOI: 10.1086/533487

Relativistic tidal properties of neutron stars
journal, October 2009


Skyrme-force parametrization: Least-squares fit to nuclear ground-state properties
journal, January 1986


Reconciliation of neutron-star masses and binding of the Λ in hypernuclei
journal, October 1991


Properties of the Binary Neutron Star Merger GW170817
journal, January 2019


A Skyrme parametrization from subnuclear to neutron star densities
journal, December 1997


Skyrme forces and giant resonances in exotic nuclei
journal, March 1999


Structure of proton drip-line nuclei around doubly magic Ni 48
journal, February 1996


Compact Stars with Sequential QCD Phase Transitions
journal, October 2017


Nonrotating and rotating neutron stars in the extended field theoretical model
journal, October 2007


The mass and the Radius of the Neutron star in the Transient Low-Mass X-Ray Binary sax J1748.9–2021
journal, February 2013


GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability
journal, September 2018


Constraints on the symmetry energy using the mass-radius relation of neutron stars
journal, February 2014


Neutron-star Radius Constraints from GW170817 and Future Detections
journal, November 2017

  • Bauswein, Andreas; Just, Oliver; Janka, Hans-Thomas
  • The Astrophysical Journal, Vol. 850, Issue 2
  • DOI: 10.3847/2041-8213/aa9994

Equation of state of nuclear matter from empirical constraints
journal, November 2014


Charge distributions of Pb 208 , Pb 206 , and Tl 205 and the mean-field approximation
journal, December 1989


Constraining the Symmetry Parameters of the Nuclear Interaction
journal, June 2013


Comparing two models for measuring the neutron star equation of state from gravitational-wave signals
journal, September 2018


Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
journal, November 2016


Asymmetric nuclear matter and neutron skin in an extended relativistic mean-field model
journal, March 2010


Constraints on a phenomenologically parametrized neutron-star equation of state
journal, June 2009


New parametrization for the Lagrangian density of relativistic mean field theory
journal, January 1997


A Skyrme parametrization from subnuclear to neutron star densities Part II. Nuclei far from stabilities
journal, May 1998


Are Small Radii of Compact Stars Ruled out by GW170817/AT2017gfo?
journal, June 2018


Generic conditions for stable hybrid stars
journal, October 2013


Constraining neutron-star tidal Love numbers with gravitational-wave detectors
journal, January 2008


Causal representations of neutron-star equations of state
journal, June 2018


GW170817: Observation of gravitational waves from a binary neutron star inspiral
text, January 2017

  • Abbott, B. P.; Abbott, R.; Abbott, T. D.
  • American Physical Society
  • DOI: 10.5167/uzh-147231

Equations of state for supernovae and compact stars
text, January 2017


Generic Conditions for Stable Hybrid Stars
conference, March 2014

  • Alford, Mark G.; Han, Sophia; Prakash, Madappa
  • Proceedings of the 12th Asia Pacific Physics Conference (APPC12)
  • DOI: 10.7566/jpscp.1.013041

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
other, January 2017

  • Abbott, B. P.; Abbott, R.; Abbott, T. D.
  • College Park : American Physical Society
  • DOI: 10.15488/4798

Properties of the Binary Neutron Star Merger GW170817
text, January 2019

  • Abbott, B. P.; Abbott, R.; Abbott, T. D.
  • College Park, MD : American Physical Society
  • DOI: 10.15488/11396

Constraining neutron star tidal Love numbers with gravitational wave detectors
text, January 2007


Non-rotating and rotating neutron stars in the extended field theoretical model
text, January 2007


Tidal Love numbers of neutron stars
text, January 2007


Constraints on a phenomenologically parameterized neutron-star equation of state
text, January 2008


Relativistic tidal properties of neutron stars
text, January 2009


Density dependence of the nuclear symmetry energy: a microscopic perspective
text, January 2009


Astrophysical Measurement of the Equation of State of Neutron Star Matter
text, January 2010


Generic conditions for stable hybrid stars
text, January 2013


Spectral Approach to the Relativistic Inverse Stellar Structure Problem II
text, January 2013


Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
text, January 2016


Masses, Radii, and Equation of State of Neutron Stars
text, January 2016


Symmetry Parameter Constraints From A Lower Bound On The Neutron-Matter Energy
text, January 2016


Compact stars with sequential QCD phase transitions
text, January 2017


Interdependence of different symmetry energy elements
text, January 2017


GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
text, January 2017


Neutron-star radius constraints from GW170817 and future detections
text, January 2017


New constraints on radii and tidal deformabilities of neutron stars from GW170817
text, January 2018


Comparing two models for measuring the neutron star equation of state from gravitational-wave signals
text, January 2018


Works referencing / citing this record:

Improved analytic modeling of neutron star interiors
journal, June 2019


Roles of crust and core in the tidal deformability of neutron stars
journal, September 2019

  • Kalaitzis, A. M.; Motta, T. F.; Thomas, A. W.
  • International Journal of Modern Physics E, Vol. 28, Issue 09
  • DOI: 10.1142/s0218301319500812

Measurement of the Nuclear Symmetry Energy Parameters from Gravitational-wave Events
journal, November 2019


A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
journal, December 2019


Improved Analytic Modeling of Neutron Star Interiors
text, January 2019