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The Maximum Mass and Rotational Kinetic Energy of Rapidly Rotating Neutron Stars

  • Authors: Shao-Peng Tang, Yong-Jia Huang, Yi-Zhong Fan

Shao-Peng Tang et al 2026 The Astrophysical Journal 1000 .

  • Provider: AAS Journals

Caption: Figure 5.

Posterior distributions of key parameters from the quarkyonic model, including the slope of symmetry energy L, the parameter Λ, the threshold density nt, and the potential parameter γ1. The values and their 68.3% credible intervals are shown for each parameter.

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