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Variation of Protoplanetary Disk Response with Adiabatic Index, Viscosity and Mass
2021
Zenodo
The protoplanetary disk is under constant perturbing forces that influences its evolution. Previous simulations studies have tried to model such a disk comprising of gas and dust for different Equation of State that completes the N- S equations solved in such a numerical approach. Along with it viscosity in the materials of such disk are studied as key parameter. We reproduced such scenarios of the disk under different host stellar mass, Kinematic viscosity 'ν' and Adiabatic Index 'γ' and found
doi:10.5281/zenodo.4566148
fatcat:areoti5525dovchwzwo2n42azu