Particle-gas dynamics in the protoplanetary nebula

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Models, Computer Programs, Gas Dynamics, Nebulae, Particle Collisions, Protoplanets, Robustness (Mathematics), Vectors (Mathematics), Astrophysics, Collision Parameters, Computerized Simulation, Flow Equations, Mathematical Models, Optimization, Turbulence, Viscosity

Scientific paper

In the past year we made significant progress in improving our fundamental understanding of the physics of particle-gas dynamics in the protoplanetary nebula. Having brought our code to a state of fairly robust functionality, we devoted significant effort to optimizing it for running long cases. We optimized the code for vectorization to the extent that it now runs eight times faster than before. The following subject areas are covered: physical improvements to the model; numerical results; Reynolds averaging of fluid equations; and modeling of turbulence and viscosity.

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