Image Details

Choose export citation format:

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 2.

Mutual friction coefficients ﹩{{ \mathcal B }}_{{\rm{co}}}﹩ as a function of normalized cylindrical radius x/Rcc for PKDD with different L0 and fixed 1.4 M neutron star mass. The shaded region indicates the range of ﹩{{ \mathcal B }}_{{\rm{co}}}﹩ for ﹩{{ \mathcal M }}_{p}^{* }/{{ \mathcal M }}_{p}=0.5﹩–0.7, with the upper and lower boundaries corresponding to ﹩{{ \mathcal M }}_{p}^{* }/{{ \mathcal M }}_{p}=0.5﹩ and ﹩{{ \mathcal M }}_{p}^{* }/{{ \mathcal M }}_{p}=0.7﹩, respectively.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse