Magnetoemission of magnetar crust


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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.

Sobre autores

V. Kondratyev

Bogolyubov Laboratory of Theoretical Physics; Universität Bielefeld

Autor responsável pela correspondência
Email: vkondrat@jinr.ru
Rússia, ul. Joliot-Curie 6, Dubna, Moscow oblast, 141980; Universitätsstraße 25, Bielefeld, 33615

Yu. Korovina

Moscow Institute of Open Education

Email: vkondrat@jinr.ru
Rússia, Prechistenskii per. 7A, Moscow, 119034

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