Analysis of molecular dynamics based chemistry models for DSMC simulation of the atmosphere of Io

Keyphrases

• Molecular Dynamics 100%
• Direct Simulation Monte Carlo 100%
• Dissociation 100%
• Monte Carlo Simulation Method 100%
• Chemistry Model 100%
• Dynamic Base 100%
• Ionian 100%
• Quasi-classical Trajectory 75%
• ReaxFF 75%
• Reaction Cross Section 50%
• Atomization 50%
• Force Field 25%
• Exchange Reaction 25%
• Atmospheric Conditions 25%
• Energy Model 25%
• Hard Spheres 25%
• Collision-induced Dissociation 25%
• Molecular Dynamics Method 25%
• Reaction Pathway 25%
• Choice Method 25%
• Low-velocity Impact 25%
• Internal Energy 25%
• Collision Model 25%
• Cross Model 25%
• Total Cross Section 25%
• Relative Velocity 25%
• Collision Energy 25%
• Sulfur Dioxide 25%
• Axisymmetric Model 25%
• Reactive Systems 25%
• Collision Cross Section 25%
• SO2 Molecule 25%
• Atmospheric Structure 25%
• Jovian Moons 25%
• Time-dependant 25%
• Molecule Dissociation 25%

Chemistry

• Chemistry 100%
• Molecular Dynamics 100%
• Monte Carlo Method 100%
• Sulfur Dioxide 100%
• Atomizer Nozzle 33%
• Collision Induced Dissociation 16%
• Collisionally Activated Dissociation (CAD) 16%
• Reaction Path 16%
• Internal Energy 16%
• Collisional 16%

Physics

• Monte Carlo Method 100%
• Molecular Dynamics 100%
• Planetary Atmosphere 100%
• Atomizing 40%
• Field Theory (Physics) 20%
• Internal Energy 20%
• Impact Velocity 20%
• Io 20%
• Atmospheric Structure 20%
• Jovian Satellites 20%
• Sulphur Dioxide 20%