• Magneto-hydrodynamic
  • Radiative transfer
  • Finite Volume Methods
  • 3D global simulations
  • HPC/GPU computing

  • Radiative transfer methods (M1)
  • Radiative hydrodynamical simulations 
  • AMR method
  • gPLUTO developer

  • MHD Jet-launching
  • Relativistic non-ideal MHD
  • PLUTO developer/non-ideal MHD methods

  • dust-gas simulations of planet disk simulations
  • synthetic observations
  • FARGO3D

  • GPU/AMR development
  • Radiative transfer/Neutrino transport
  • gPLUTO/AthenaK
  • HPC/GPU computing

  • Radiation hydrodynamic
  • Dust methods
  • Radiative transfer
  • HPC computing

  • Radiative hydrodynamical simulations 
  • Accretion bursts
  • Gas opacities
  • HPC computing

  • Hydrodynamical simulations with gas/dust drag
  • Streaming instability
  • Particle + fluid dust methods
  • HPC computing

  • MagnetoHydrodynamical simulations
  • Magnetic driven winds
  • Ambipolar diffusion
  • HPC computing

  • MagnetoHydrodynamical simulations
  • Inner disk/Magnetic winds
  • Embedded planets
  • HPC computing

  • MagnetoHydrodynamical simulations
  • Planet-disk interaction
  • Circumplanetary disks
  • gPLUTO

  • Radiative transfer
  • Circumplanetary disk
  • RADMC3D

  • Hydrodynamical simulations 
  • Vertical shear instability
  • Dust particle motion
  • HPC computing

  • Radiation Hydrodynamical simulations
  • Dust fluid methods
  • Radiative transfer – FLD methods
  • HPC computing