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- W1615320897 abstract "Dissipation of magnetic fields in Hall plasma of neutron star crusts may power persistent high energy emission of a class of strongly magnetized neutrons stars, magnetars. We consider development of a dissipative tearing mode in Hall plasma (electron MHD) and find that its growth rate increases with the wave number of perturbations, reaching a maximum value intermediate between resistive $tau_r$ and Hall times $tau_H$, $Gammasim 1 / sqrt{tau_r tau_H}$. We argue that the tearing mode may be the principal mechanism by which strong magnetic fields are dissipated in magnetars on times scale of $sim 10^4-10^5$ yrs powering the persistent X-ray emisison." @default.
- W1615320897 created "2016-06-24" @default.
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- W1615320897 date "2007-05-22" @default.
- W1615320897 modified "2023-09-27" @default.
- W1615320897 title "Dissipation of magnetic fields in neutron star crusts due to development of a tearing mode" @default.
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