MD simulations identify a universal post-break plastic flow in neutron star crusts at shear strains of 0.05-0.11, independent of initial crystal structure.
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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.
citing papers explorer
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Plasticity of Neutron Star Crusts
MD simulations identify a universal post-break plastic flow in neutron star crusts at shear strains of 0.05-0.11, independent of initial crystal structure.
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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.