Abstract
The magnetoemission of crusts of magnetars (ultramagnetized neutron stars) is considered as an origin of repeated soft gamma-ray bursts. It is shown that all observations of such bursts can be described and systematized on the basis of amodel of randomly jumping interacting moments that includes quantum fluctuations and internuclear magnetic interaction in inhomogeneous crusty nuclear matter.
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Kondratyev, V.N., Korovina, Y.V. Magnetoemission of magnetar crust. Phys. Atom. Nuclei 80, 558–561 (2017). https://doi.org/10.1134/S1063778817030139
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DOI: https://doi.org/10.1134/S1063778817030139