期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 453, 期 1, 页码 581-590出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv1642
关键词
conduction; dense matter; stars: neutron
资金
- Russian Science Foundation [14-12-00316]
- Russian Science Foundation [14-12-00316] Funding Source: Russian Science Foundation
We present a simplemodel for electron transport in a possible layer of exotic nuclear clusters (in the so-called nuclear pasta layer) between the crust and liquid core of a strongly magnetized neutron star. The electron transport there can be strongly anisotropic and gyrotropic. The anisotropy is produced by different electron effective collision frequencies along and across local symmetry axis in domains of exotic ordered nuclear clusters and by complicated effects of the magnetic field. We also calculate averaged kinetic coefficients in case local domains are freely oriented. Possible applications of the obtained results and open problems are outlined.
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