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Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact

  • Authors: Keiya Murashima, Takanori Sasaki

Keiya Murashima and Takanori Sasaki 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 20.

Rock and ice components in the disk as a function of Limp. Left panel: baseline simulations utilizing the Wendland C6 kernel and approximately 105 particles. Middle panel: test for the kernel choice using the Wendland C2 kernel with N ≈ 105 particles. Right panel: test for spatial resolution using N ≈ 106 particles and the Wendland C6 kernel.

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