Viscous Dissipation and Heat Conduction in Binary Neutron-Star Mergers
Viscous Dissipation and Heat Conduction in Binary Neutron-Star Mergers
Inferring the properties of dense matter is one of the most exciting prospects from the measurement of gravitational waves from neutron star mergers. However, it requires reliable numerical simulations that incorporate viscous dissipation and energy transport as these can play a significant role in the survival time of the post-merger …