First simulations of neutron star evolution with the BDNK formulation produce stable evolutions in a restricted parameter space and permit analysis of quasi-normal mode frequencies and fundamental mode decay rates.
Continuum and Discrete Initial-Boundary-Value Problems and Ein- stein’s Field Equations.Living Rev
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Neutron star evolution with the Bemfica-Disconzi-Noronha-Kovtun viscous hydrodynamics framework
First simulations of neutron star evolution with the BDNK formulation produce stable evolutions in a restricted parameter space and permit analysis of quasi-normal mode frequencies and fundamental mode decay rates.