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Title: 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
 [1]; ORCiD logo [2]
  1. Shandong Univ., Weihai (China); Texas A & M Univ., Commerce, TX (United States); Texas A&M University-Commerce
  2. Texas A & M Univ., Commerce, TX (United States)

Here, what can we learn about the density dependence of nuclear symmetry energy $${E}_{\mathrm{sym}}(\rho)$$ from precise measurements of the radius (R1.4) and/or tidal polarizability (Λ1.4) of canonical neutron stars with a mass of 1.4 $${{\rm{M}}}_{\odot }$$? With the $${E}_{\mathrm{sym}}(\rho)$$ parameterized using three parameters L, Ksym, and Jsym which have the asymptotic meaning of being respectively the slope, curvature, and skewness of symmetry energy at saturation density, we found that, while both the R1.4 and Λ1.4 depend strongly on the slope L, the Ksym and Jsym parameters characterizing the high-density behavior of $${E}_{\mathrm{sym}}(\rho)$$ also play appreciable roles. Thus, there is not a simple relation between the Λ1.4/R1.4 and L alone. Precise measurements of just the Λ1.4 and R1.4 cannot completely determine the $${E}_{\mathrm{sym}}(\rho)$$ but limit combinations of its parameters. In particular, stringent constraints approximately independent of the Jsym on the L–Ksym correlations can be obtained. However, infinite combinations of the larger (smaller) L and smaller (larger) Ksym can lead to the same Λ1.4 and R1.4. Additional observables including those from terrestrial nuclear experiments are thus necessary to break this degeneracy in order to completely determine the density dependence of nuclear symmetry energy $${E}_{\mathrm{sym}}(\rho)$$.

Research Organization:
Texas A & M Univ., Commerce, TX (United States)
Sponsoring Organization:
National Natural Science Foundation of China (NNSFC); USDOE Office of Science (SC), Nuclear Physics (NP)
Grant/Contract Number:
SC0009971; SC0013702
OSTI ID:
1658237
Journal Information:
Journal of Physics. G, Nuclear and Particle Physics, Journal Name: Journal of Physics. G, Nuclear and Particle Physics Journal Issue: 1 Vol. 46; ISSN 0954-3899
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (11)

High-density nuclear symmetry energy extracted from astrophysical observations
  • Li, Bao-An; Krastev, P. G.; Wen, De-Hua
  • 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
conference January 2019
Constraining compact star properties with nuclear saturation parameters journal July 2019
Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules journal 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 journal September 2019
Consistent relativistic mean-field models constrained by GW170817 journal April 2019
Extracting nuclear symmetry energies at high densities from observations of neutron stars and gravitational waves journal March 2019
Towards understanding astrophysical effects of nuclear symmetry energy journal July 2019
Possible maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model journal August 2019
Constraining compact star properties with nuclear saturation parameters text January 2019
Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules text 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 text January 2019