English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Thermal conductivity and shear viscosity of npe$\mu$ matter in non-superfluidneutron star cores are considered in the framework of Brueckner-Hartree-Fockmany-body theory. We extend our previous work (Shternin, Baldo and Haensel,2013) by analysing different nucleon-nucleon potentials and differentthree-body forces. We find that the use of different potentials leads up to oneorder of magnitude variations in the values of the nucleon contribution totransport coefficients. The nucleon contribution dominates the thermalconductivity, but for all considered models the shear viscosity is dominated byleptons.

Transport coefficients in neutron star cores in BHF approach. Comparison of different nucleon potentials