Numerical model of fast electron energy loss in H2 finds 11% of energy to direct ro-vibrational excitation and 1.5-2 times higher yields for high-vibrational states via electronic cascading than earlier Monte Carlo calculations.
Atomic Data and Nuclear Data Tables , year = 2021, month = jul, volume =
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Numerical model of fast electron energy deposition in interstellar molecular gas
Numerical model of fast electron energy loss in H2 finds 11% of energy to direct ro-vibrational excitation and 1.5-2 times higher yields for high-vibrational states via electronic cascading than earlier Monte Carlo calculations.