The kinetic scheme, build in the past for the investigation of the vibrational kinetics of the ground electronic state in low-pressure negative ion sources and in the radiative-coupled simulation of entry conditions in the Jupiter atmosphere, has been improved including the H+ 3, H- ion kinetics, and the detailed dynamics of the electron-impact excitation of singlet states of H2 molecule (B, B? 1? u , C, D 1?u) [1] resolved on both initial and final vibrational manifolds, together with the de-excitation channels, i.e. the radiative decay and the collisional quenching, and also accounting for the VT and VV collisional processes responsible for the redistribution of energy between vibrational and translational degrees of freedom. The state-to-state kinetic simulation has been carried out with the GPKin code that couples self-consistently a set of master equations describing the time evolution of the chemical species (atomic and molecular) densities and their internal (electronic and vibrational) distributions and the Boltzmann equation for the electron energy distribution function, eedf, taking into account the external electric field. The state-to-state self-consistent approach, implementing the detailed kinetic scheme, has been exploited for the simulation of non-equilibrium conditions in nanosecond repetitively pulsed discharges in pure hydrogen [2], in H2/N2 plasma [3], of interest for the investigation on nitrogen seeding experiments in tokamak divertor and in H2/He plasma [4], of interest for the interpretation of shock tube experiments for atmospheric entry of gaseous giant planets. The chemical model for H2/Li plasma is under construction, including the electron impact induced processes in LiH [5], for the interest in liquid metal divertors.
State-to-state self-consistent kinetic modelling of hydrogen plasmas
Laricchiuta A;Pietanza LD;Capitelli M;Colonna G
2021
Abstract
The kinetic scheme, build in the past for the investigation of the vibrational kinetics of the ground electronic state in low-pressure negative ion sources and in the radiative-coupled simulation of entry conditions in the Jupiter atmosphere, has been improved including the H+ 3, H- ion kinetics, and the detailed dynamics of the electron-impact excitation of singlet states of H2 molecule (B, B? 1? u , C, D 1?u) [1] resolved on both initial and final vibrational manifolds, together with the de-excitation channels, i.e. the radiative decay and the collisional quenching, and also accounting for the VT and VV collisional processes responsible for the redistribution of energy between vibrational and translational degrees of freedom. The state-to-state kinetic simulation has been carried out with the GPKin code that couples self-consistently a set of master equations describing the time evolution of the chemical species (atomic and molecular) densities and their internal (electronic and vibrational) distributions and the Boltzmann equation for the electron energy distribution function, eedf, taking into account the external electric field. The state-to-state self-consistent approach, implementing the detailed kinetic scheme, has been exploited for the simulation of non-equilibrium conditions in nanosecond repetitively pulsed discharges in pure hydrogen [2], in H2/N2 plasma [3], of interest for the investigation on nitrogen seeding experiments in tokamak divertor and in H2/He plasma [4], of interest for the interpretation of shock tube experiments for atmospheric entry of gaseous giant planets. The chemical model for H2/Li plasma is under construction, including the electron impact induced processes in LiH [5], for the interest in liquid metal divertors.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.