arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2407.03212cond-mat.quant-gasastro-ph.HEhep-ph
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利用偶极超固体探索脉冲星周期突变

Exploring pulsar glitches with dipolar supersolids

Thomas Bland, Francesca Ferlaino, Massimo Mannarelli, Elena Poli, Silvia Trabucco

AI总结:

本研究借助中子星内壳层与偶极超固体的相似性,数值分析涡旋俘获机制及物质密度分布对脉冲星周期突变的影响,为实验室天体量子模拟奠定基础。

摘要:

周期突变是打断旋转中子星逐渐自转减慢过程的突发自转加速事件。学界认为它们由中子星内壳层中涡旋的快速脱钉引发。中子星内壳层与偶极超固体之间的相似性为研究周期突变提供了途径。借助该相似性,我们数值分析了涡旋俘获机制以及物质密度分布如何影响周期突变。这些结果为在实验室中开展天体的量子模拟铺平了道路。

英文摘要:

Glitches are sudden spin-up events that interrupt the gradual spin-down of rotating neutron stars. They are believed to arise from the rapid unpinning of vortices in the neutron star inner crust. The analogy between the inner crust of neutron stars and dipolar supersolids allows to investigate glitches. Employing such analogy, we numerically analyze the vortex trapping mechanism and how the matter density distribution influences glitches. These results pave the way for the quantum simulation of celestial bodies in laboratories.

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。

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