Our Team

- Magneto-hydrodynamic
- Radiative transfer
- Finite Volume Methods
- 3D global simulations
- HPC/GPU computing
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- Radiative transfer methods (M1)
- Radiative hydrodynamical simulations
- AMR method
- gPLUTO developer
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- MHD Jet-launching
- Relativistic non-ideal MHD
- PLUTO developer/non-ideal MHD methods
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- dust-gas simulations of planet disk simulations
- synthetic observations
- FARGO3D
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- GPU/AMR development
- Radiative transfer/Neutrino transport
- gPLUTO/AthenaK
- HPC/GPU computing
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- Radiation hydrodynamic
- Dust methods
- Radiative transfer
- HPC computing
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- Radiative hydrodynamical simulations
- Accretion bursts
- Gas opacities
- HPC computing
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- Hydrodynamical simulations with gas/dust drag
- Streaming instability
- Particle + fluid dust methods
- HPC computing
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- MagnetoHydrodynamical simulations
- Magnetic driven winds
- Ambipolar diffusion
- HPC computing
- More

- MagnetoHydrodynamical simulations
- Inner disk/Magnetic winds
- Embedded planets
- HPC computing
- More

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