Relativistic electron impact ionization cross sections of carbon ions and application to an optically thin plasma. (arXiv:1909.08370v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Avillez_M/0/1/0/all/0/1">Miguel A. de Avillez</a> (1,2), <a href="http://arxiv.org/find/astro-ph/1/au:+Guerra_M/0/1/0/all/0/1">Mauro Guerra</a> (3), <a href="http://arxiv.org/find/astro-ph/1/au:+Santos_J/0/1/0/all/0/1">José Paulo Santos</a> (3), <a href="http://arxiv.org/find/astro-ph/1/au:+Breitschwerdt_D/0/1/0/all/0/1">Dieter Breitschwerdt</a> (2) (1) <a href="http://arxiv.org/find/astro-ph/1/au:+Evora_U/0/1/0/all/0/1">University of Évora</a> (Portugal), (2) <a href="http://arxiv.org/find/astro-ph/1/au:+Berlin_T/0/1/0/all/0/1">Technical University Berlin</a> (Germany), (3) <a href="http://arxiv.org/find/astro-ph/1/au:+Lisbon_N/0/1/0/all/0/1">New University of Lisbon</a> (Portugal)
Aims. Determination of K- and L-shell cross sections of the carbon atom and
ions using the modified relativistic binary encounter Bethe (MRBEB) method, a
simple analytical scheme based on one atomic parameter that allows determining
electron-impact ionization cross sections. The quality of the cross sections
calculated with the MRBEB method is shown through: (i) comparison with those
obtained with the general ionization processes in the presence of electrons and
radiation (GIPPER) code and the flexible atomic code (FAC), and (ii)
determination of their effects on the ionic structure and cooling of an
optically thin plasma.
Results. The three sets of cross sections show deviations among each other in
different energy regions. The largest deviations occur near and in the peak
maximum. Ion fractions and plasma emissivities of an optically thin plasma that
evolves under collisional ionization equilibrium, derived using each set of
cross sections, show deviations that decrease with increase in temperature and
ionization degree. In spite of these differences, the calculations using the
three sets of cross sections agree overall. Conclusions. A simple model like
the MRBEB is capable of providing cross sections similar to those calculated
with more sophisticated quantum mechanical methods in the GIPPER and FAC codes.
Aims. Determination of K- and L-shell cross sections of the carbon atom and
ions using the modified relativistic binary encounter Bethe (MRBEB) method, a
simple analytical scheme based on one atomic parameter that allows determining
electron-impact ionization cross sections. The quality of the cross sections
calculated with the MRBEB method is shown through: (i) comparison with those
obtained with the general ionization processes in the presence of electrons and
radiation (GIPPER) code and the flexible atomic code (FAC), and (ii)
determination of their effects on the ionic structure and cooling of an
optically thin plasma.
Results. The three sets of cross sections show deviations among each other in
different energy regions. The largest deviations occur near and in the peak
maximum. Ion fractions and plasma emissivities of an optically thin plasma that
evolves under collisional ionization equilibrium, derived using each set of
cross sections, show deviations that decrease with increase in temperature and
ionization degree. In spite of these differences, the calculations using the
three sets of cross sections agree overall. Conclusions. A simple model like
the MRBEB is capable of providing cross sections similar to those calculated
with more sophisticated quantum mechanical methods in the GIPPER and FAC codes.
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