Simple electron-impact excitation cross-sections including plasma density effects
Autor: | Jean-Christophe Pain, Djamel Benredjem |
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Rok vydání: | 2021 |
Předmět: |
Nuclear and High Energy Physics
Atomic Physics (physics.atom-ph) Plane wave FOS: Physical sciences 01 natural sciences Physics - Atomic Physics 010305 fluids & plasmas symbols.namesake Pauli exclusion principle 0103 physical sciences Radiative transfer Coulomb 010306 general physics Quantum Solar and Stellar Astrophysics (astro-ph.SR) Physics Radiation Physics - Plasma Physics Computational physics Numerical integration Plasma Physics (physics.plasm-ph) Astrophysics - Solar and Stellar Astrophysics symbols Atomic physics Degeneracy (mathematics) Bessel function |
Zdroj: | High Energy Density Physics. 38:100923 |
ISSN: | 1574-1818 |
DOI: | 10.1016/j.hedp.2021.100923 |
Popis: | The modeling of non-local-thermodynamic-equilibrium plasmas is crucial for many aspects of high-energy-density physics. It often requires collisional-radiative models coupled with radiative-hydrodynamics simulations. Therefore, there is a strong need for fast and as accurate as possible calculations of the cross-sections and rates of the different collisional and radiative processes. We present an analytical approach for the computation of the electron-impact excitation (EIE) cross-sections in the Plane Wave Born (PWB) approximation. The formalism relies on the screened hydrogenic model. The EIE cross-section is expressed in terms of integrals, involving spherical Bessel functions, which can be calculated analytically. In order to remedy the fact that the PWB approximation is not correct at low energy (near threshold), we consider different correcting factors (Elwert-Sommerfeld, Cowan-Robb, Kilcrease-Brookes). We also investigate the role of plasma density effects such as Coulomb screening and quantum degeneracy on the EIE rate. This requires to integrate the collision strength multiplied by the Fermi-Dirac distribution and the Pauli blocking factor. We show that, using an analytical fit often used in collisional-radiative models, the EIE rate can be calculated accurately without any numerical integration, and compare our expression with a correction factor presented in a recent work. Comment: submitted to High Energy Density Phys |
Databáze: | OpenAIRE |
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