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GW190814's Secondary Component with Mass 2.50–2.67 M as a Superfast Pulsar

  • Authors: Nai-Bo Zhang and Bao-An Li

2020 The Astrophysical Journal 902 38.

  • Provider: AAS Journals

Caption: Figure 4.

Examples of the density dependence of nuclear symmetry energy predicted by nuclear many-body theories using different interactions, energy density functionals, and/or techniques in comparison with the constraining boundaries extracted from studying properties of neutron stars (the upper/lower thick blue line corresponds to the left/right green boundaries shown in Figure 3).

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