期刊
ASTROPHYSICAL JOURNAL
卷 833, 期 2, 页码 -出版社
IOP Publishing Ltd
DOI: 10.3847/1538-4357/833/2/189
关键词
dense matter; magnetic fields; stars: magnetars; stars: neutron; waves
资金
- Monash Research Acceleration grant, NASA [NNX13AI34G]
- Simons Foundation [446228]
We explore the interaction between Hall waves and mechanical failures inside a magnetar crust, using detailed one-dimensional models that consider temperature-sensitive plastic flow, heat transport, and cooling by neutrino emission, as well as the coupling of the crustal motion to the magnetosphere. We find that the dynamics is enriched and accelerated by the fast, short-wavelength Hall waves that are emitted by each failure. The waves propagate and cause failures elsewhere, triggering avalanches. We argue that these avalanches are the likely sources of outbursts in transient magnetars.
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