Λཻࢠ i ͱཻࢠ j ͷཧྔΛೖྗͱͨ͠ࡍͷ Star region Ͱͷѹྗͷͱͯ͠ Pix N ∑ j UiUj q2 i vij · ∇iWij(hi) = N ∑ j P∗ ij UiUj q2 i vij · ∇iWij(hi), (10) ͕Γཱͭͱఆٛ͢Δɻ • P∗ ij Λཻࢠ i ཻ͕ࢠ j ͔Βड͚Δѹྗͷ࣌ؒฏۉྔͱ͢Δɻ ౬ઙ (ஜେֶ) Godunov DISPH ଔۀݚڀൃදձ, January 31, 2023 11 / 17
scheme)” created by Jlcercos is licenced under CC BY-SA 4.0(https://creativecommons.org/licenses/by-sa/4.0/) ౬ઙ (ஜେֶ) Godunov DISPH ଔۀݚڀൃදձ, January 31, 2023 17 / 17
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discontinuities and kelvin–helmholtz instabilities in sph. Journal of Computational Physics, 227(24):10040–10057. [Saitoh and Makino, 2013] Saitoh, T. R. and Makino, J. (2013). A DENSITY-INDEPENDENT FORMULATION OF SMOOTHED PARTICLE HYDRODYNAMICS. The Astrophysical Journal, 768(1):44. [Wadsley et al., 2017] Wadsley, J. W., Keller, B. W., and Quinn, T. R. (2017). Gasoline2: a modern smoothed particle hydrodynamics code. Monthly Notices of the Royal Astronomical Society, 471(2):2357–2369. ౬ઙ (ஜେֶ) Godunov DISPH ଔۀݚڀൃදձ, January 31, 2023 17 / 17