Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 453, Issue 1, Pages 581-590Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv1642
Keywords
conduction; dense matter; stars: neutron
Categories
Funding
- Russian Science Foundation [14-12-00316]
- Russian Science Foundation [14-12-00316] Funding Source: Russian Science Foundation
Ask authors/readers for more resources
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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available