Transport parameters in neutron stars from in-medium N N cross sections
Data(s) |
2010
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Resumo |
We present a numerical study of shear viscosity and thermal conductivity of symmetric nuclear matter, pure neutron matter, and beta-stable nuclear matter, in the framework of the Brueckner theory. The calculation of in-medium cross sections and nucleon effective masses is performed with a consistent two- and three-body interaction. The investigation covers a wide baryon density range as needed in the applications to neutron stars. The results for the transport coefficients in beta-stable nuclear matter are used to make preliminary predictions on the damping time scales of nonradial modes in neutron stars. |
Identificador | |
Idioma(s) |
英语 |
Fonte |
Zhang, HF; Lombardo, U; Zuo, W.Transport parameters in neutron stars from in-medium N N cross sections,PHYSICAL REVIEW C ,2010,82(1):15805 |
Palavras-Chave | #NUCLEAR-MATTER #FERMI LIQUID #DENSE NUCLEAR #3-BODY FORCE #SUPERFLUIDITY #VISCOSITY #HE-3 |
Tipo |
期刊论文 |