The giant impact simulations with density independent smoothed particle hydrodynamics

@inproceedings{Hosono2016TheGI,
  title={The giant impact simulations with density independent smoothed particle hydrodynamics},
  author={Natsuki Hosono and Takayuki R. Saitoh and Junichiro Makino and Hidenori Genda and Shigeru Ida},
  year={2016}
}
Abstract At present, the giant impact (GI) is the most widely accepted model for the origin of the Moon. Most of the numerical simulations of GI have been carried out with the smoothed particle hydrodynamics (SPH) method. Recently, however, it has been pointed out that standard formulation of SPH (SSPH) has difficulties in the treatment of a contact discontinuity such as a core–mantle boundary and a free surface such as a planetary surface. This difficulty comes from the assumption of… CONTINUE READING
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