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Constraint on the symmetry energy at high densities from neutron star observations using relativistic mean-field models

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In this paper, we constrain the symmetry energy at high densities in nuclear matter using recent observations of neutron stars based on the calculations of relativistic mean-field (RMF) models.

Description

Using the observations of the neutron stars, we obtain the constraint on the symmetry energy at high densities, S(2ρ0) = 40.54±12.47MeV, and S(3ρ0) = 44.12±29.38MeV.

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Provenance · 1 source records, 11 field assertions
SourceKeyLast seenRaw
ScienceDB10.57760/sciencedb.j00186.0066312 d agoJSON v1
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