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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 8.

Neutron star mass as a determining factor in glitch characteristics. (a) Higher-mass neutron stars exhibit suppressed overshoot and smaller glitch steps. (b) The corresponding timing residuals show distinct mass-dependent signatures, particularly in the overshoot region.

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