后闪期中子星性质与地壳运动
Neutron Stars Properties and Crust Movements in Post-glitch Epoch
摘要：
利用一种新的非均匀自适应网格数值计算程序，研究了后毛刺时期地壳物质运动对中子星整体性质的影响。我们的数值分析表明，这些变化可能有助于解释所观察到的旋转频率的自旋下降。
英文摘要：
Using a new numerical code with non-uniform adapted mesh, we study the changes produced in the global properties of neutron stars by the motion of matter in crust region during post-glitch epoch. Our numerical analysis shows that these changes may contribute to explain the observed spin-down of rotational frequency.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
