SPH simulations find that disk mass and size after a Uranus-forming impact are robust to EOS choice while rock fraction is highly sensitive.
and Reinhardt, Christian and Meier, Matthias M
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A review of SPH modeling for global-scale impacts, emphasizing material properties across size regimes and links to Solar System observations.
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Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact
SPH simulations find that disk mass and size after a Uranus-forming impact are robust to EOS choice while rock fraction is highly sensitive.
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Recent advances in modelling of global-scale collisions using smoothed particle hydrodynamics
A review of SPH modeling for global-scale impacts, emphasizing material properties across size regimes and links to Solar System observations.