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Delineating effects of nuclear symmetry energy on the radii and tidal polarizabilities of neutron stars

Journal Article · · Journal of Physics. G, Nuclear and Particle Physics

Not provided.

Research Organization:
Texas A & M Univ., Commerce, TX (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
DOE Contract Number:
SC0009971; SC0013702
OSTI ID:
1611281
Journal Information:
Journal of Physics. G, Nuclear and Particle Physics, Vol. 46, Issue 1; ISSN 0954-3899
Publisher:
IOP Publishing
Country of Publication:
United States
Language:
English

References (46)

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral October 2017
Multi-messenger Observations of a Binary Neutron Star Merger October 2017
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Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State April 2018
Neutron Skins and Neutron Stars in the Multimessenger Era April 2018
New Constraints on Radii and Tidal Deformabilities of Neutron Stars from GW170817 June 2018
Tidal Deformability from GW170817 as a Direct Probe of the Neutron Star Radius April 2018
Critical examination of constraints on the equation of state of dense matter obtained from GW170817 October 2018
GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability September 2018
Neutron Star Tidal Deformabilities Constrained by Nuclear Theory and Experiment August 2018
Tidal Love Numbers of Neutron Stars April 2008
Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral June 2010
Nuclear Constraints on Properties of Neutron star Crusts May 2009
Neutron Star Equation of State from the Quark Level in Light of GW170817 July 2018
Combined Constraints on the Equation of State of Dense Neutron-rich Matter from Terrestrial Nuclear Experiments and Observations of Neutron Stars May 2018
Constraining the radii of neutron stars with terrestrial nuclear laboratory data November 2006
Neutron Star Structure and the Equation of State March 2001
Topical issue on nuclear symmetry energy February 2014
Neutron Skin of Pb 208 , Nuclear Symmetry Energy, and the Parity Radius Experiment June 2011
Skyrme interaction and nuclear matter constraints March 2012
Relativistic mean-field hadronic models under nuclear matter constraints November 2014
Isospin Physics in Heavy-Ion Collisions at Intermediate Energies April 1998
Reaction dynamics with exotic nuclei May 2005
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Elliptic flow and the Symmetry Energy at Supra-Saturation Density June 2012
Constraints on the symmetry energy and neutron skins from experiments and theory July 2012
A way forward in the study of the symmetry energy: experiment, theory, and observation July 2014
The nuclear symmetry energy November 2016
Symmetry Parameter Constraints from a Lower Bound on Neutron-matter Energy October 2017
How tightly is the nuclear symmetry energy constrained by a unitary Fermi gas? November 2017
Equations of state for supernovae and compact stars March 2017
Constraining the neutron–proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density November 2013
Asymmetric nuclear matter equation of state November 1991
Deducing the nuclear-matter incompressibility coefficient from data on isoscalar compression modes September 2006
Do we understand the incompressibility of neutron-rich matter? May 2010
Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817 November 2017
Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars January 2018
Neutron star matter at sub-nuclear densities June 1973
The Ground State of Matter at High Densities: Equation of State and Stellar Models November 1971
Symmetry Energy of Dilute Warm Nuclear Matter May 2010
Effects of the liquid-gas phase transition and cluster formation on the symmetry energy February 2014
Diffusive instability of a kaon condensate in neutron star matter December 2004
Nuclear symmetry energy and stability of matter in neutron stars August 2007
Neutron star observations: Prognosis for equation of state constraints April 2007

Cited By (11)

High-density nuclear symmetry energy extracted from astrophysical observations
  • No authors listed
  • XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY, AIP Conference Proceedings https://doi.org/10.1063/1.5117808
January 2019
Constraining compact star properties with nuclear saturation parameters July 2019
Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules August 2019
Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state September 2019
Consistent relativistic mean-field models constrained by GW170817 April 2019
Extracting nuclear symmetry energies at high densities from observations of neutron stars and gravitational waves March 2019
Towards understanding astrophysical effects of nuclear symmetry energy July 2019
Possible maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model August 2019
Constraining compact star properties with nuclear saturation parameters January 2019
Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules January 2019
Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state January 2019

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