This paper presents approximate correction factors to collisional excitation and ionisation rates which account for special relativity in the free electron motion as a function of free electron temperature and the threshold energy of the reaction. These are calculated by taking the ratio of collisional rates derived from simple empirical cross sections using relativistic and non-relativistic mechanics. These results are extended to de-excitation and three body recombination rates using detailed balance. It is found that the relativistic correction is significant in regimes potentially important to galactic intracluster media and diagnostic dopants in burning ICF plasmas
Reliably interpreting spectra from both photoionized and electron-ionized cosmic plasmas re-quires a...
International audienceWe have investigated the effects of a non-thermal electron population on the i...
An accurate knowledge of atomic collision processes is important for a better understanding of many ...
This paper presents approximate correction factors to collisional excitation and ionisation rates wh...
Collisional-radiative models enable average ionization and ionization populations, plus the rates of...
We show that while corrections to spectroscopically measured Franck-Condon energies, arising from mo...
The general relativistic kinetic theory is applied to calculate corrections to the distribution aris...
A study is made of the problem of describing the cosmological expansion of a plasma in the framework...
Dielectronic recombination is the dominant process by which free electrons recombine with ions in as...
In this work we introduce a new expression of the plasma Dielecronic Recombination (DR) rate as a fu...
An exact solution is obtained to the nonrelativistic Focker-Planck equation for electrons at the Com...
One of the most crucial steps for a fast ignition scenario is the energy deposition into the highly ...
High temperature plasmas are ubiquitous in high energy astrophysics and are becoming increasingly ac...
The purpose of this thesis is to study magnetic reconnection in collisionless and relativistic plasm...
This thesis investigates ultra-relativistic processes of thermal production of electrons and positro...
Reliably interpreting spectra from both photoionized and electron-ionized cosmic plasmas re-quires a...
International audienceWe have investigated the effects of a non-thermal electron population on the i...
An accurate knowledge of atomic collision processes is important for a better understanding of many ...
This paper presents approximate correction factors to collisional excitation and ionisation rates wh...
Collisional-radiative models enable average ionization and ionization populations, plus the rates of...
We show that while corrections to spectroscopically measured Franck-Condon energies, arising from mo...
The general relativistic kinetic theory is applied to calculate corrections to the distribution aris...
A study is made of the problem of describing the cosmological expansion of a plasma in the framework...
Dielectronic recombination is the dominant process by which free electrons recombine with ions in as...
In this work we introduce a new expression of the plasma Dielecronic Recombination (DR) rate as a fu...
An exact solution is obtained to the nonrelativistic Focker-Planck equation for electrons at the Com...
One of the most crucial steps for a fast ignition scenario is the energy deposition into the highly ...
High temperature plasmas are ubiquitous in high energy astrophysics and are becoming increasingly ac...
The purpose of this thesis is to study magnetic reconnection in collisionless and relativistic plasm...
This thesis investigates ultra-relativistic processes of thermal production of electrons and positro...
Reliably interpreting spectra from both photoionized and electron-ionized cosmic plasmas re-quires a...
International audienceWe have investigated the effects of a non-thermal electron population on the i...
An accurate knowledge of atomic collision processes is important for a better understanding of many ...