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A Microphysical Probe of Neutron Star Interiors: Constraining the Equation of State with Glitch Dynamics

  • Authors: Zhonghao Tu, Ang Li

Zhonghao Tu and Ang Li 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

(a) Crustal superfluid angular velocity (﹩{{\rm{\Omega }}}_{{\rm{sf}}}^{{\rm{cr}}}﹩) and (b) core superfluid angular velocity (﹩{{\rm{\Omega }}}_{{\rm{sf}}}^{{\rm{co}}}﹩) as a function of the normalized cylindrical radius and time following a glitch. The gray solid vertical line marks the radial position of the crust–core interface in the equatorial plane. The effective interaction PKDD with L0 = 40 MeV, effective mass ﹩{m}_{n}^{* }/{m}_{n}=1.0﹩, and neutron star mass 1.4 M are adopted.

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