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- W2510363636 abstract "Neutron stars are ideal astrophysical laboratories for testing theories of the de Haas–van Alphen effect and diamagnetic phase transition which is associated with magnetic domain formation. The magnetic interaction between delocalized magnetic moments of electrons (the Shoenberg effect), can result in an effect of the diamagnetic phase transition into domains of alternating magnetization (Condon's domains). Associated with the domain formation are prominent magnetic field oscillation and anisotropic magnetic stress which may be large enough to fracture the crust of magnetar with a super-strong field. Even if the fracture is impossible as in low-field magnetar, the depinning phase transition of domain wall (DW) motion driven by low field rate (mainly due to the Hall effect) in the randomly perturbed crust can result in a catastrophically variation of magnetic field. This intermittent motion, similar to the avalanche process, makes the Hall effect be dissipative. These qualitative consequences about magnetized electron gas are consistent with observations of magnetar emission, and especially the threshold critical dynamics of driven DW can partially overcome the difficulties of low-field magnetar bursts and the heating mechanism of transient, or outbursting magnetar." @default.
- W2510363636 created "2016-09-16" @default.
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- W2510363636 date "2016-08-29" @default.
- W2510363636 modified "2023-10-18" @default.
- W2510363636 title "The Diamagnetic Phase Transition of Dense Electron Gas: Astrophysical Applications" @default.
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- W2510363636 doi "https://doi.org/10.1088/1538-3873/128/968/104201" @default.
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