Seminal molecular dynamics results on neutron star crust breaking are non-converged and require strain rates slower than 10^{-5} times the plasma frequency with N≈10^5 particles for convergence.
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Revisiting the Rheology of Neutron Star Crusts with Molecular Dynamics
Seminal molecular dynamics results on neutron star crust breaking are non-converged and require strain rates slower than 10^{-5} times the plasma frequency with N≈10^5 particles for convergence.