This paper presents a method for estimating the pressure variance at the inner edge of a neutron star crust. The obtained results quantify uncertainty in the estimation of pressure at the core-crust interface, implying that they depend on the selected equation of state and the neutron star's mass distribution function. The quality of the transition pressure determination depends on the neutron star's mass, with a significant decrease in accuracy for configurations with masses close to $2\mathrm{M}\odot$. The method used makes it possible to control the theoretical part of the core-crust pressure dispersion in determining the observational quantities.

中文翻译：

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中子星壳内缘压力的分散

本文提出了一种估计中子星壳内缘压力变化的方法。获得的结果量化了核心-地壳界面压力估计的不确定性，这意味着它们取决于所选的状态方程和中子星的质量分布函数。过渡压力确定的质量取决于中子星的质量，质量接近$2\mathrm{米}\odot$. 所使用的方法可以在确定观测量时控制岩心-地壳压力分散的理论部分。