Exploring pulsar glitches with dipolar supersolids
arXiv:2407.03212 · doi:10.1007/s00601-024-01949-7
Abstract
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.
18 pages, 8 figures
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Cited by in corpus (6)
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- Anomalous dispersion of shear waves in dipolar supersolids
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