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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 1.

High-density behavior of nuclear symmetry energy Esym(ρ) (top panel) and the corresponding isospin asymmetry profile δ(ρ) in NSs at β equilibrium (bottom panel) as functions of the reduced baryon density ρ/ρ0 by varying the parameter Jsym within its broad range predicted by nuclear theories while all other EOS parameters are fixed at the values indicated. Taken from Zhang et al. (2018).

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