http://arxiv.org/abs/1711.06520
Understanding signals from neutron stars requires knowledge about the transport inside the star. We review the transport properties and the underlying reaction rates of dense hadronic and quark matter in the crust and the core of neutron stars and point out open problems and future directions.
A. Schmitt and P. Shternin
Mon, 20 Nov 17
50/56
Comments: 71 pages; commissioned for the book “Physics and Astrophysics of Neutron Stars”, NewCompStar COST Action MP1304