Electron-neutron scattering and transport properties of neutron stars
We show that electrons can couple to the neutron excitations in neutron stars and find that this can limit their contribution to the transport properties of dense matter, especially the shear viscosity. The coupling between electrons and neutrons is induced by protons in the core, and by ions in the...
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Veröffentlicht in: | arXiv.org 2014-09 |
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Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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